The galaxy presents as a single, concentrated luminous object. Its morphology appears largely smooth and elliptical, with a high degree of central concentration of light. The overall shape is consistent with a rounded structure rather than a highly flattened disk.

The color appears to be primarily yellow-orange, suggestive of an older stellar population. The lack of prominent blue hues or distinct spiral arm features indicates a relatively low rate of ongoing star formation. There is no obvious indication of tidal tails, merging features, or significant morphological disturbance, suggesting a relatively quiescent state.
