The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of roundness. There is a distinct central bulge that appears more yellow in color, indicating a higher concentration of older stars. Extending outwards from the core, the galaxy exhibits a fainter and slightly bluer halo, suggesting the presence of a younger stellar population. The overall structure appears relatively undisturbed, although subtle irregularities in the outer regions suggest a possible history of minor interactions or accretion events. No prominent spiral arms or distinct dust lanes are visible. The galaxy is estimated to have a moderate stellar mass and a low rate of star formation.
