The galaxy presents as a centrally concentrated, smooth, and nearly circular object. The light profile appears to be dominated by a bulge component, exhibiting a gradual decrease in surface brightness from the core outwards. A slight ellipticity is present, but it is nearly round in appearance. There is no discernible spiral arm structure or prominent dust lanes visible. The dominant color is yellow, suggesting a stellar population of older stars, consistent with a relatively low ongoing star formation rate. No evidence of major mergers or tidal disturbances are obvious within the available image resolution.
