The galaxy presents as a somewhat elliptical, disk-like structure with a noticeable central bulge. The core region exhibits a concentrated luminosity gradient, suggesting a significant stellar density. Moving outward from the core, the galactic disk appears relatively smooth in texture. A faint hint of spiral structure may be present, though it is not distinctly resolved. The overall color profile suggests a mix of stellar populations, with the central region appearing yellower, which could indicate older, redder stars and potentially dust obscuration. The outer regions display a bluer hue, which is indicative of younger, hotter stars and regions of active star formation. There is a small asymmetry, suggesting a possible minor interaction or disturbance. There is no clear evidence of a major ongoing merger or significant tidal features.
