The galaxy presents a complex morphology, exhibiting a disturbed or irregular structure indicative of possible interaction or merging events. The overall shape appears elongated, with a notable central concentration that transitions into a diffuse outer region.

Color gradients are apparent within the galaxy. The core region exhibits a yellowish-white hue, potentially indicating an older stellar population or significant dust obscuration. The outer regions display a bluer tint, suggesting the presence of younger, hotter stars. This bluer component appears patchy and unevenly distributed, giving the impression of active star formation regions interspersed within a more evolved stellar population.

There is evidence of asymmetry in the galaxy's structure. One side appears more extended or distorted than the other, possibly influenced by tidal forces from a past or ongoing interaction. Faint extensions or streams of material seem to emanate from the main body, further supporting the hypothesis of gravitational disturbance.
