The galaxy appears to be a relatively smooth, rounded object, showing characteristics of an elliptical galaxy. There is a slight indication of some asymmetry in the galaxy's profile. The central region of the galaxy exhibits a concentrated luminosity profile, fading towards the outer edges. There is no prominent evidence of spiral arm structure or significant dust lanes. The overall color suggests an older stellar population. A small disturbance or minor merging event cannot be ruled out, but the dominant impression is that of a relaxed, well-established system.
