This galaxy presents as a moderately bright, elliptical-like structure. The central region exhibits a high concentration of light, appearing smooth and diffuse with a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the light intensity decreases gradually, and the color shifts towards a slightly bluer tone, hinting at the presence of younger, hotter stars possibly within a faint disk-like structure. The overall shape is slightly elongated, not perfectly spherical, but with no clear spiral arms or bar features discernible. There might be some minor disturbances or asymmetries in the outer regions, suggesting past interactions or mergers, though it is predominantly a smooth, consolidated system.
