The galaxy presents as a concentrated, largely featureless elliptical or lenticular system. Its overall morphology appears smooth, with no immediately discernible spiral arms or bar structure. The light distribution appears centrally concentrated, with a gradual falloff in surface brightness towards the outer regions. The galaxy has a slightly elliptical shape, appearing close to circular but with a minor elongation.

In color, the galaxy exhibits a yellowish-orange hue, which implies an older stellar population with a lower rate of ongoing star formation, and may contain a population of older red giant stars. There is no evidence of significant dust lanes or patches of intense blue star formation regions, further supporting the interpretation of a passively evolving system with little active star birth. There is no visual evidence of major mergers or tidal disturbances, and the galaxy appears relatively undisturbed. There is also no indication of a strong active galactic nucleus in the core.
