The galaxy presents a largely elliptical morphology, exhibiting a smooth and concentrated central bulge. There is a notable lack of prominent spiral arms or distinct disk features. The galaxy displays a yellowish-white hue centrally, suggesting a population dominated by older stars. Fainter, reddish tinges can be observed offset slightly from the central region, potentially indicating areas of dust obscuration or the presence of cooler, redder stellar populations. Overall, the galaxy appears relatively undisturbed, without obvious signs of major ongoing mergers or tidal interactions.
