The galaxy presents as a smooth, centrally concentrated object. The light distribution appears relatively uniform across the galaxy's body, with no distinct spiral arms or bar structures readily apparent. It exhibits an elliptical morphology. There is some evidence of minor disturbances in the light distribution, possibly indicating a minor interaction. The color suggests a population of older stars and minimal ongoing star formation. Based on the color and morphology, the galaxy is likely to be a massive elliptical galaxy.
