The galaxy presents as a slightly elongated, elliptical or lenticular structure, displaying a relatively smooth morphology. The central bulge is prominent and appears brighter than the surrounding disk or halo, with a concentrated luminosity profile. The overall color is suggestive of an older stellar population, and there's no obvious spiral arm structure or prominent dust lanes visible in this imagery. Some slight asymmetry may be present in the outer regions, possibly indicating a minor gravitational disturbance or past interaction. There does not appear to be an active galactic nucleus. The size appears relatively compact.
