The galaxy presents an elliptical morphology, with a smooth and diffuse light profile. A concentrated nucleus is present exhibiting a red hue, potentially indicative of an older stellar population within the galactic center. The overall color gradient transitions from reddish at the core to a bluer periphery, which may indicate a radial distribution of stellar ages with younger stars concentrated in the outer regions. There's a minor asymmetrical distribution of light suggesting possible past interactions, or mergers; however, the smooth nature of the galaxy suggests the effects of such an encounter have largely subsided. The galaxy appears relatively isolated, showing no obvious signs of ongoing major merger activity or tidal disruption.
