The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth, diffuse profile with no readily apparent spiral arm structure or prominent dust lanes. The core is bright and gradually fades into the surrounding halo, which is yellowish in color. The high central concentration and lack of disk features suggest it may be an early-type galaxy. The galaxy's apparent color indicates an older stellar population with diminished recent star formation. The object exhibits minimal tidal disturbances or evidence of ongoing mergers in the main body of the galaxy.