The galaxy exhibits a flattened elliptical morphology, appearing as a smooth, centrally concentrated distribution of light. Its intermediate roundness suggests a classification between perfectly spherical and highly elongated. There is no visible evidence of strong tidal disturbances or major mergers. Minor asymmetries are present, possibly indicating a recent minor interaction or internal dynamical processes. The galaxy has a slightly higher concentration of light at the center which emits yellowish light, which could indicate older stars. The outer disk-like region emits a slightly bluish light, which could indicate younger stars.
