The galaxy appears to be relatively compact and exhibits a smooth, elliptical morphology. Its central region shows a concentrated luminosity gradient, suggestive of a prominent galactic nucleus. The color profile indicates a redder central region, potentially indicative of an older stellar population. The outer regions fade gradually into the background, with little evidence of spiral arms or significant substructure. There is a subtle hint of a possible extended halo, but its boundaries are poorly defined in this image. The overall structure appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. Minor distortions are possible. The galaxy appears largely spheroidal and well rounded.
