This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a gradual decrease in brightness towards the outer regions. The morphology suggests minimal disk-like structure or prominent spiral arms. There is a slight elongation to its shape, appearing somewhere between a round and cigar shape. There is no evidence of any major merging events or significant tidal disturbances, though very minor disturbances can't be ruled out. Color gradients suggest that the central region is populated by older stars, indicated by the redder color. The outer regions appear slightly bluer, suggestive of ongoing star formation.
