The galaxy presents as a largely homogenous, elliptical-appearing structure. It exhibits a high degree of central concentration, characterized by a bright, yellowish-white core region that gradually fades into the surrounding halo. The halo is diffuse and relatively smooth, with a subtle gradient in surface brightness extending outwards. No distinct spiral arms or prominent dust lanes are discernible within the observed morphology. The overall color suggests a population of older stars, with a relatively low rate of current star formation activity. There are some subtle disturbances visible in the outer halo, suggesting past interactions with smaller galaxies. The shape appears to be close to circular, with only slight indications of elongation. Overall, this galaxy appears to be an early-type galaxy, potentially an elliptical, in a relatively quiescent state.
