This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that dominates the overall luminosity. There is a noticeable color gradient, with the core appearing more yellow-white, suggesting an older stellar population. The outer regions of the galaxy transition towards a redder hue, also indicative of older stars and potentially a lower rate of ongoing star formation in these regions. The galaxy lacks any discernible spiral arms or prominent dust lanes. Its morphology appears undisturbed, showing no strong evidence of recent major mergers or tidal interactions, although there may be minor disturbances to the right side of the image.
