The galaxy presents as a fairly smooth, centrally concentrated object. There is a lack of readily apparent spiral arm structure or a distinct disk component; the light appears relatively uniform across the galaxy's face. There is very little evidence of tidal tails or streams, and the overall morphology indicates a low probability of recent major mergers. It exhibits a predominantly rounded shape, showing a slight deviation from being perfectly circular. The color profile suggests a moderate age stellar population. The relatively muted color, exhibiting minimal blue component, indicates that the galaxy's rate of star formation is relatively low.
