The galaxy presents as a relatively smooth, centralized object with a discernible but not highly pronounced disk-like structure. Its overall shape is somewhat elliptical, appearing more rounded than elongated. The light distribution is concentrated towards the center, suggesting a significant bulge component.

There's evidence of a color gradient, with the central bulge exhibiting a yellowish-red hue, possibly indicative of an older stellar population. The outer regions of the disk show a bluer tint, implying the presence of younger, hotter stars and ongoing star formation.

No strong tidal features or major disturbances are apparent, suggesting the galaxy is relatively undisturbed. There is, however, some minor asymmetry in the outer regions, hinting at possible past interactions or internal dynamical processes. The galaxy appears generally isolated, with no obvious signs of a major merger or ongoing interaction with another large system.
