The galaxy presents a generally smooth morphology. It has a roughly round shape, with a slight elongation. A central, brighter bulge region is visible, indicative of a concentration of older stars. There is a fainter disk component surrounding the bulge. The galaxy exhibits a bluish hue, particularly in the outer regions, suggesting the presence of some younger stars. The overall structure doesn't appear significantly disturbed, although there might be some minor asymmetry or subtle distortions. There does not appear to be a merging event occurring.
