The galaxy presents as an elliptical morphology, appearing smooth and with a high degree of central concentration. Its shape deviates noticeably from a perfect circle, exhibiting a moderate elongation resembling an in-between shape rather than a purely round or cigar-shaped form. The color gradient transitions from a reddish-orange core to a greenish-blue outer halo. There are no prominent spiral arm structures or significant dust lanes visible. The galaxy does not show any signs of major ongoing mergers or significant tidal disturbances, though subtle asymmetries or minor disturbances are not entirely absent. The overall appearance suggests a relatively evolved system, potentially an early-type galaxy with a relatively quiescent star formation history. The distribution of light indicates the presence of a considerable population of older stars concentrated toward the center, with a slightly younger stellar population and/or low-level star formation activity in the outer regions.
