The galaxy appears to be a lenticular or early-type spiral, with a smooth, centralized bulge dominating its structure. There is a slight elongation suggesting it is not perfectly spherical, perhaps leaning toward a cigar shape. The disk is faint and shows little evidence of distinct spiral arms or active star formation. The overall color is yellowish-white, indicating an older stellar population with a lower rate of current star formation, and is a moderate-sized galaxy, neither exceptionally large nor particularly small. There is no obvious visual evidence of tidal disturbances or ongoing merger activity.
