The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light distribution. The core is a bright yellowish-white hue, indicative of an older stellar population. Progressing outward, the color shifts towards a more greenish-yellow, possibly reflecting the presence of younger stars or ongoing star formation, though less pronounced compared to spiral galaxies. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. There is a slight asymmetry of the galaxy with one side having slightly less concentrated light distribution. The overall structure suggests a system dominated by evolved stars.
