The galaxy presents a generally smooth, elliptical morphology. The light profile appears highly concentrated toward the center, exhibiting a bright, yellowish core region. This central concentration suggests a substantial bulge component. Moving outward from the core, the galaxy fades gradually into a more diffuse halo. There is no distinct disk structure or prominent spiral arm features visible. The galaxy's color suggests a population of older stars with lower levels of ongoing star formation. There may be some minor disturbances present in the halo structure. The overall shape appears close to round.
