The galaxy presents as a roughly elliptical, diffuse structure. Its color profile suggests an older stellar population, with a concentration of yellower, possibly redder stars towards the central bulge. The outer regions exhibit bluer hues, potentially indicating some ongoing, albeit limited, star formation. There is evidence of a disk structure with a slight inclination towards our line of sight. The galaxy doesn't exhibit any major distortions or tidal features, and appears relatively undisturbed, although minor asymmetry may be present. Overall, it is most likely an early-type spiral galaxy or an elliptical galaxy with a weak star formation rate.
