The galaxy presents as a centrally concentrated, lenticular structure. It appears largely featureless, with a smooth luminosity gradient extending outwards from a bright, yellow-hued core. A very faint, diffuse disk component appears to be present, exhibiting a slightly bluer color than the core, suggestive of modest ongoing star formation. The overall shape is closer to round than elongated but is neither completely spherical nor highly flattened. There is no obvious evidence of major morphological disturbance or recent merger events. The light profile indicates a relatively evolved stellar population dominating the central regions.
