The galaxy appears as a centrally concentrated, smooth object with a predominantly elliptical morphology. The light profile exhibits a gradual decline in intensity from the center outwards, lacking any distinct spiral arm structures or prominent features indicative of active star formation regions. The galaxy's color appears to be reddish-orange, suggesting a population of older stars and a relatively low rate of on-going star formation, with dust likely playing a role in reddening the light. There is a very slight indication of a possible minor disturbance in its symmetry, but it is largely a relaxed system. It is a massive galaxy.
