The galaxy presents as a single, concentrated light source. Its morphology is dominated by a smooth, spheroidal structure. The light profile appears relatively uniform, lacking any distinct spiral arms or a prominent disk. The color is slightly yellowish, indicating a population of older stars, and suggesting a low current rate of star formation. There may be a very faint hint of a surrounding halo, but it is not well defined. No signs of recent or ongoing major mergers are apparent, but very subtle disturbances cannot be ruled out. The galaxy has a generally circular appearance.