The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. Its color profile suggests a population dominated by older stars, resulting in a yellowish-red hue. There is no discernible dust lane or spiral arm structure. The galaxy appears fairly symmetrical and undisturbed, showing no obvious signs of a recent major merger or interaction with other galaxies. There may be some indication of minor disturbances. The estimated size indicates that it is a sizable galaxy. Low star formation activity is suggested based on color.
