The galaxy appears as a centrally concentrated, yellowish-white object. It exhibits a generally smooth morphology, with no immediately discernible spiral arms or bar structures. The overall shape approximates a sphere, although there might be a slight ellipticity. Color gradients suggest that the central regions are dominated by older stellar populations, and potentially, dust absorption. There appears to be only a faint extended halo, and there is no evidence of ongoing major mergers or significant tidal distortions in the immediate vicinity. The lack of strong blue emission suggests that the galaxy is in a relatively quiescent phase of star formation. There may be some low-level star formation occurring.
