The galaxy presents as a centrally concentrated object with a largely smooth morphology. The overall shape appears to be elliptical or lenticular, exhibiting a moderate degree of ellipticity. A dominant, bright core is evident, transitioning into a slightly fainter, extended halo or bulge. No distinct spiral arms or bar structures are discernible within the observed light distribution. The color profile indicates a generally redder hue, potentially indicative of an older stellar population and relatively low levels of ongoing star formation activity. There is no apparent indication of tidal disturbances, close companions, or any signs of a major ongoing merger event. Subtle irregularities might be present in the outer regions of the galaxy, hinting at minor disturbances, but they are not prominent.
