The galaxy presents a largely elliptical morphology with a smooth, concentrated central bulge. It exhibits a general yellow-red color profile, suggesting an older stellar population, though hints of blue-green near the edges suggest the presence of some younger stars. The galaxy's smooth appearance indicates a lack of prominent spiral arms or significant dust lanes, consistent with an early-type galaxy undergoing little to no active star formation. The overall light distribution is highly centralized with a relatively quick decline in surface brightness away from the core. There is no obvious evidence of recent merger activity or tidal disturbances in the immediate vicinity of the galaxy.
