The galaxy presents a mixed morphology, displaying characteristics of both elliptical and potentially spiral structures. The central region exhibits a bright, smooth component, appearing largely spheroidal. Extending outward from this central bulge, there is a fainter, more diffuse structure that suggests the presence of a disk, although its features are indistinct.

There's evidence of possible tidal disturbance or interaction with another galaxy. An irregular shape and the presence of faint wisps of light extending away from the main body might indicate past or ongoing interactions with smaller companions. A small portion of this galaxy seems to have a tidal bridge with a close, point-like object, which could be indicative of some form of merging. The central bulge has a slight elongated shape.

Color gradients suggest variations in stellar populations across the galaxy. The central bulge tends towards yellow/orange, indicative of older, redder stellar populations.

Overall, the galaxy exhibits a complex structure, with indications of a relatively smooth central component and disk with disturbed or interacting features, suggesting that the galaxy is not fully relaxed or isolated. Additional observations are needed to determine more details about its components and evolutionary history.