The galaxy presents as a relatively smooth, elliptical-like object with no obvious spiral arm structures or a well-defined disk. It appears centrally concentrated with a gradual decrease in luminosity extending outwards from the core. The color is predominantly yellowish, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is little evidence of dust lanes or prominent HII regions. The overall appearance is consistent with a massive galaxy that has largely ceased active star formation. There are no signs of any major ongoing merger activity, although a minor disturbance cannot be completely ruled out based on the image.
