The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. It displays a somewhat elongated morphology, significantly more cigar shaped than round. There are no readily apparent spiral arms or distinct features indicative of active star formation in the visible bands. The dominant color is on the redder end of the spectrum, suggesting an older stellar population. No signs of major mergers or significant tidal disturbances are observed. Light appears fairly consistent across the surface, without any distinct knots, or regions of higher density. The galaxy appears fairly isolated.
