The galaxy appears as a slightly elliptical, centrally concentrated object. The light distribution is smooth, with no obvious spiral arm structures or distinct features. The color gradient suggests a population of older stars, likely dominated by redder wavelengths. There is a hint of a diffuse outer halo surrounding the central bulge, but its boundaries are poorly defined in this image. Overall, the galaxy presents a morphology consistent with an early-type galaxy. There's no visible indication of ongoing mergers or significant tidal disturbances.
