The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a high degree of radial symmetry. The light distribution suggests a bulge-dominated morphology. The core exhibits a bright, yellowish-white color, potentially indicating an older stellar population. Moving outwards, the color gradually shifts to a slightly bluer hue, possibly signaling the presence of some younger stars, although the overall star formation rate appears to be relatively low. There is no obvious spiral structure or bar. Minor asymmetries or tidal features are not readily apparent, suggesting it is a relatively undisturbed galaxy.
