The galaxy presents an elliptical morphology. The central bulge exhibits a bright, yellowish-white luminosity, suggesting a significant population of older stars. A faint, diffuse halo of bluish light surrounds the core, which transitions into the darker background. This may indicate the presence of younger, bluer stars in the outer regions, though their relative number is small. Some faint, irregular structures are observed in the outer regions of the galaxy, which may imply minor gravitational interactions or disturbances with other galaxies. Overall, the galaxy exhibits a smooth appearance. Star formation is low. The galaxy is relatively massive.
