The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and yellow-orange in color, which appears to be smoothly merging with the outer regions. The shape tends towards being in between round and elliptical, with a slight elongation. There is minimal evidence of spiral arm structure or significant dust lanes within the visible light spectrum. Faint indications of minor disturbances may exist within the galaxy's outer halo but could also be artifacts. There is no indication of significant recent or ongoing mergers. The estimated size is approximately 6 kpc in radius. The galaxy's color suggests a population of older stars, indicating a relatively low rate of current star formation.
