The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright central bulge that exhibits a yellowish hue, indicative of a population of older stars. The light gradually decreases outwards from the center. There are hints of bluer regions in the outer parts of the galaxy, possibly suggesting areas of more recent star formation. The overall shape appears close to round, with no obvious signs of significant tidal disturbances or ongoing major mergers, although there might be some minor irregularity or slight asymmetries present.
