The galaxy presents as a relatively smooth, centrally concentrated structure with a mostly elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar. There is a subtle color gradient from a slightly bluer core region outwards to a redder halo or outer disk. The galaxy's light profile indicates a high degree of central symmetry, with no obvious signs of major tidal disturbances or ongoing mergers, though subtle disturbances or minor interactions cannot be ruled out. The lack of significant blue light and the presence of redder colors suggest a population dominated by older stars and a low rate of current star formation. The galaxy appears relatively isolated.
