This galaxy presents a largely smooth morphology. It exhibits a centrally concentrated luminosity profile, with a bright, well-defined core that gradually fades into the outer regions. The overall shape appears spheroidal, exhibiting a high degree of roundness. There is no readily apparent disk structure, spiral arms, or bar features discernible in the image. The color profile suggests a population of older stars dominating the central region. The image does not indicate any ongoing major merging events or significant tidal disturbances. Faint outer features indicate some minor disturbances. The galaxy is comparatively small but has an absolute magnitude that places it as fairly luminous. Very low star formation is expected within the galaxy.
