The galaxy presents an elliptical morphology. The core region is luminous, appearing primarily reddish, suggesting a population of older stars. Moving outward from the core, the galaxy's color shifts towards a bluer hue, indicating the presence of a younger stellar population in the outer regions. There is no clear dust lane or spiral arm structure evident in this image, hinting that star formation occurs at a relatively low rate. The galaxy displays a fairly smooth overall appearance with no significant disturbances or tidal features visible, suggesting that it has not undergone a major merger recently, although there might be signs of a minor disturbance. The estimated size of the galaxy indicates that it is reasonably massive and extended.
