The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that is an orange-yellow color. Moving outwards from the center, there is a gradual decrease in the intensity of the light with a redder hue. It shows little evidence of spiral arm structure. A very faint disk may be present, but not much dust is visible. There are some minor irregularities in its shape, suggesting a possible recent or ongoing minor interaction. There is no prominent tidal tail or shell structure visible to indicate a major merger. The color suggests a relatively older stellar population and low star formation activity.
