The galaxy presents as a moderately luminous, elongated structure, likely an elliptical galaxy at an approximate distance corresponding to a redshift of 0.12. It exhibits a smooth, centralized concentration of light, suggesting an older stellar population with minimal recent star formation. The shape is notably cigar-shaped.

Faint diffuse emissions surround the central core, potentially indicating an extended halo of older stars or tidally stripped material. The overall structure appears relatively undisturbed. There is a low incidence of any significant ongoing merger activity.
