The galaxy presents as an elliptical or lenticular system, appearing largely featureless with a smooth light distribution. The central region exhibits a concentrated, bright core which fades towards the edges. There is a slight elongation, and appears to have a moderate degree of sphericity. No distinct spiral arm structure is visible, however, some faint, diffuse, patchy regions of bluer light may suggest limited ongoing star formation. There is no evidence of tidal tails or significant morphological disturbances, indicating a relatively settled state. The red-yellow color index indicates a dominant population of older stars.
