The galaxy appears as a relatively smooth, centrally concentrated object. Its shape is generally elliptical, deviating slightly from a perfect circle. A subtle color gradient is visible; the central region exhibits a yellow hue, transitioning to a bluer tint towards the outer edges. This color difference potentially indicates variations in stellar populations, with younger, bluer stars residing in the periphery, and older, redder stars dominating the core. There is no obvious spiral structure or prominent dust lanes visible in the galaxy. There is a slight possibility of minor tidal disturbances, but this is difficult to assess based on the image. It may be a result of the galaxy's morphology. Overall, the galaxy appears to be an early-type galaxy exhibiting characteristics of relatively high age.
