The galaxy presents as a slightly elongated, lenticular-like structure, displaying a relatively smooth, symmetrical light distribution. There is no apparent spiral arm structure or significant dust lane features visible. The primary color gradient is a redder central bulge transitioning to a slightly bluer, though still relatively quiescent, outer region. This coloration suggests an older stellar population dominating the central region with potentially some ongoing, but limited, star formation in the outer areas. The object does not appear to be undergoing any significant mergers or tidal disruptions.
