The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decrease in surface brightness outwards from the core. The central region appears yellowish, suggesting a dominant population of older stars. Surrounding the core, there is a bluer halo, possibly indicating a younger stellar population or some ongoing star formation activity. The overall shape appears moderately elliptical, with a suggestion of a disk-like component, although no spiral arms are clearly resolved. There is no obvious evidence of any major merging activity or significant tidal disturbances. There is a slight asymmetry in the outer regions of the galaxy.
