The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. The core exhibits a yellowish-orange hue, indicative of an older stellar population. The outer regions transition to a bluer color, suggesting the presence of some younger stars, but overall star formation activity appears to be relatively low. The galaxy lacks any apparent spiral arm structures or significant dust lanes. The shape appears largely elliptical, trending towards circular, with no obvious signs of tidal disruption or recent merger events, with a very slight irregularity to one side. There are some faint red features to the bottom side of the galaxy.
