The galaxy presents a generally smooth and rounded morphology. The light distribution is dominated by a central bulge that exhibits a concentrated, yellowish-white hue. There is evidence of a surrounding disk, although it appears relatively featureless with a somewhat muted greenish tint. The galaxy does not show any obvious signs of spiral arm structure or significant dust lanes. Its color profile suggests a population of older stars. There are no obvious signs of tidal disturbances or ongoing major mergers.