The galaxy presents an elliptical morphology, exhibiting a dominant, smooth central bulge. The isophotes appear moderately flattened, displaying an intermediate ellipticity between round and cigar-shaped. A faint disk-like structure is discernable surrounding the bulge. There are signs of a possible interaction or disturbance given the slight elongation and asymmetry. The galaxy exhibits colors consistent with an older stellar population. The apparent size indicates a substantial physical extent.
