The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy given its overall form. It exhibits a moderate ellipticity, appearing somewhat elongated along one axis. The light profile suggests a bulge-dominated morphology, with a strong central concentration of luminosity that gradually decreases with increasing radius. There is a color gradient visible from the core outwards. The central region is relatively bright, with a yellowish-white hue. Moving outward, the color shifts to a slightly redder tone. No distinct spiral arm features or prominent dust lanes are observed. The galaxy's overall color suggests a population of older stars, indicative of relatively low current star formation.