The galaxy presents as a moderately luminous, elliptical structure. Its overall morphology is predominantly smooth, with a high degree of central concentration of light. There is a slight elongation and very little evidence of spiral arms or significant disk structure. The color profile suggests a population of older stars, contributing to the overall yellowish hue. Subtle irregularities in the outer regions suggest past minor interactions or disturbances, but the galaxy appears largely undisturbed. It has a high mass and a modest rate of star formation.
