The galaxy presents as a relatively compact and luminous object. It appears to be generally smooth in texture, with a somewhat elliptical morphology. No spiral arm structures are readily discernible. The galaxy exhibits a centrally concentrated luminosity profile. The color gradient suggests an older stellar population, generally consistent with an early-type galaxy. There may be some slight distortion or asymmetry in its shape, potentially indicating a past or ongoing interaction, but the overall structure appears largely undisturbed. There is a slight chance of there being a very weak disk. Overall, the galaxy appears to be a massive system, located at a considerable distance.
