The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which is the brightest region of the galaxy. The light distribution appears centrally condensed. There is no obvious presence of spiral arms or a prominent disk. There is some suggestion of a slight asymmetry or minor perturbation in the outer halo regions. The color profile of the galaxy suggests a population of older stars, as it is more yellow/red in appearance, with little evidence of ongoing star formation, or any significant blue regions. The overall shape is very close to round.
