The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a bright nucleus that fades gradually towards the edges. There is some indication of a disk-like structure, but it is not strongly defined. The galaxy exhibits a roughly round shape. There are no obvious signs of a major merger event, though there is a subtle asymmetry in the light distribution that could possibly indicate minor disturbances. There may be some evidence of ongoing star formation, although the galaxy's red color suggests that it is likely composed of older stars.
