The object appears to be a relatively smooth galaxy with a slight elongation, somewhere between round and cigar-shaped. There is no distinct disk structure or spiral arms visible. The galaxy exhibits a centrally concentrated luminosity profile, fading gradually towards its outer edges, with the highest intensity being a yellowish-white color. There does not appear to be evidence of significant recent mergers or major disturbances to the galactic structure. A slight irregularity in the light distribution, or a possible minor disturbance, is suggested at the lower edge of the galaxy. Overall, the galaxy presents as a largely undisturbed system dominated by evolved stellar populations.
