The galaxy presents a largely smooth morphology, with a notable central bulge. There is faint suggestion of a surrounding disk. The shape is approximately elliptical, showing deviation from a perfectly circular form. The color profile suggests a population of older stars in the bulge. The overall structure does not appear to be significantly disturbed, with no obvious signs of major mergers or tidal interactions. The faint color gradient extending outward indicates a diminishing stellar population in the outer regions.
