The galaxy presents a largely smooth, somewhat elliptical morphology, appearing more rounded than elongated. A central bulge region is visible, exhibiting a slightly more concentrated light profile compared to the surrounding galactic disk or halo. The overall color of the galaxy appears slightly bluer towards the outer regions, which could imply recent or ongoing star formation. No distinct spiral arm structures or strong tidal features are readily apparent, suggesting a relatively undisturbed system. There is a subtle indication of minor disturbances, possibly related to interactions, that could be affecting the morphology and star formation activity. The color indices suggest a moderately luminous galaxy with an estimated stellar mass indicative of a large system.
