The galaxy appears as a moderately luminous, relatively compact object. Its morphology is largely smooth and elliptical, with a dominant, spheroidal component. There are hints of some structural features or disk-like qualities, but these are not prominent. The light distribution suggests a centrally concentrated profile. The color indices indicate a population of older stars, with a relatively low rate of star formation inferred, and a considerable mass. The galaxy shows no obvious signs of major mergers or significant disturbances. The shape tends towards rounder, with cigar shapes being relatively rare.
