The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. There is little evidence of spiral arms or distinct disk features. The primary color appears to be a yellowish-orange, suggesting an older stellar population and a relative lack of ongoing, significant star formation. There is a subtle color gradient, with the central region appearing more intensely orange, potentially indicating a higher density of older stars or dust obscuration in that area. The galaxy is compact and has a fairly regular shape, with no obvious signs of major mergers or tidal disturbances.
