The galaxy presents as a relatively smooth, elliptical morphology. It appears largely featureless with no discernable spiral arms or bar structure. The central bulge is prominent and exhibits a yellowish hue, suggesting a population of older stars. The outer regions appear fainter and slightly bluer, possibly indicating some ongoing, though limited, star formation activity. There is no evidence of significant dust lanes or tidal disturbances, suggesting the galaxy is relatively undisturbed. The galaxy shows a general round appearance. There is no indication of any major merging activity.
