The galaxy appears to be a relatively compact system. Its shape is somewhat elongated, exhibiting a cigar-like appearance, although a slight asymmetry is noted. The light profile is concentrated towards the center, suggesting a significant bulge component.

Color gradients are evident within the galaxy. The central region appears to be dominated by yellow and orange hues, indicative of an older stellar population. The outer regions show hints of bluer colors, which could suggest the presence of younger stars or ongoing star formation, although this is less pronounced.

There is an indication of a possible minor disturbance in the galaxy's structure, perhaps suggesting a past or ongoing interaction with another galaxy, or a minor internal disruption. The overall impression is that this galaxy is in a transition phase, possibly evolving from a disk-dominated to a bulge-dominated system. The system does not appear to be undergoing a major merger, although there is a possibility of less intense interactions.
