The galaxy appears to be an elliptical galaxy with a generally smooth, round morphology. Its core region presents a concentrated, bright yellowish-white luminosity, suggesting a population of older stars. Surrounding the core, the galaxy exhibits a diffuse halo that gradually fades into the background. The halo shows hints of blueish color interspersed throughout, potentially indicating some presence of younger stellar populations or ongoing star formation. No distinct spiral arms or a prominent disk structure are discernible. There are no obvious signs of tidal disturbances or recent mergers, but the galaxy doesn't appear perfectly symmetrical, with some slightly uneven distribution of light in the halo region. Overall, the galaxy exhibits characteristics of a relatively evolved system.
