The galaxy presents a somewhat irregular morphology, possibly indicative of an ongoing or past interaction. The galaxy exhibits a smooth central bulge that transitions into more diffuse and disturbed outer regions. There are two primary color components visible. The central region displays a yellowish-orange hue, indicative of an older stellar population with lower ongoing star formation. The outer regions display a bluer tint, possibly due to the presence of younger stars or the effects of dust scattering. The galaxy's light profile suggests it is relatively compact, with most of its luminosity concentrated in the central region. Faint tidal features, such as faint streamers or asymmetries, might be present but are not readily apparent given the image resolution. Overall, the galaxy is likely a massive, relatively quiescent system experiencing a possible minor merger or tidal interaction, with some ongoing low-level star formation activity.
