The galaxy exhibits a generally smooth morphology, appearing as an elliptical-like structure. Its core presents a concentrated, bright, yellowish hue, which gradually fades into a less intense greenish-blue halo. The light distribution suggests a higher density of older stellar populations in the central region, with a possible presence of younger, hotter stars in the outer regions, indicated by the faint bluish tint. The shape is not perfectly spherical, appearing slightly elongated or in between. There are no distinct spiral arms, bar structures, or dust lanes visible. Overall, the galaxy appears relatively undisturbed, with no major signs of tidal interactions or mergers. Faint irregularities may suggest minor disturbances.
