The galaxy presents as a relatively smooth, spheroidal object. It exhibits a concentrated central bulge with a fairly sharp decline in luminosity moving outward. The color profile is predominantly reddish-orange, suggesting an older stellar population and/or significant dust obscuration. There is a subtle hint of green around the perimeter of the galaxy. The object appears nearly circular, with no obvious signs of a disk structure or spiral arms. There is no evidence of a major merger, though a small satellite galaxy cannot be ruled out, and the overall appearance is that of an early-type galaxy. The galaxy has a high mass estimate, but low star formation rate.
