The galaxy presents as a roughly circular, diffuse object. It exhibits a smooth, elliptical morphology with no apparent spiral arm structure or significant dust lanes visible. The central region shows a concentrated, bright core, indicative of a possible galactic bulge. Color gradients suggest the presence of a relatively old stellar population, with a yellowish-red hue dominating the galaxy's overall color. There is no obvious evidence of ongoing major star formation, though faint blue tinges at the edge of the galaxy suggest there could be some recent star formation occurring. No signs of major merging activity or significant tidal disturbances are apparent in the immediate vicinity of the galaxy.
