The galaxy presents a generally elliptical morphology, appearing largely featureless with a smooth light distribution. There is a distinct central bulge, appearing brighter and more concentrated than the surrounding galactic disk. The light profile suggests a centrally concentrated spheroid. Subtle color variations are present, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions show a bluer tint, suggesting the presence of some younger stars. There is no strong evidence of spiral arms or a bar structure. The overall shape is close to circular, with a slightly elongated appearance.
