The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge that transitions smoothly outward. Its overall morphology lacks any obvious spiral arm structures or prominent dust lanes. The dominant color appears yellowish, suggesting a population of older stars with lower ongoing star formation rates. There is a hint of bluer light within the galaxy's periphery. This may indicate the presence of a younger stellar population, though the degree of star formation activity is low overall. There is no obvious evidence of recent or ongoing major mergers or tidal disturbances affecting its overall shape. Its form is close to round.
