The galaxy exhibits a generally smooth morphology, appearing elliptical in shape, with a high degree of central concentration. The light profile indicates a relatively featureless structure, with a possible bulge component dominating the central region.  There is little evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. A subtle color gradient is observed, with the central region appearing more yellowish, suggesting an older stellar population, while the outer regions exhibit a slightly bluer hue. The overall color suggests ongoing, but moderate, star formation activity.
