The galaxy presents as a diffuse, elliptical-like structure, with a somewhat irregular shape. The central region exhibits a higher surface brightness, suggesting a concentrated nucleus. The overall color profile appears relatively red, possibly indicative of an older stellar population with ongoing or recent star formation. There is evidence of possible tidal disturbances, or a close companion. These disturbances hint at past or ongoing gravitational interactions. The spatial extent of the galaxy is estimated to be several kiloparsecs. The galaxy is mostly smooth, with a slightly disturbed structure.
