The galaxy presents as a centrally concentrated, yellowish object. It exhibits a generally smooth appearance with no immediately discernible spiral arm structure or prominent dust lanes. The isophotes appear roughly circular, suggesting a minimal degree of ellipticity. There are no clear signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity. Given the smooth morphology, it is possibly an elliptical galaxy. The color suggests a population of older stars. Given its relatively low star formation rate, it appears to be a relatively quiescent system. The galaxy's absolute magnitude indicates that this is a luminous object, a relatively large and massive system.
