The galaxy presents a mixed morphological profile. The primary component appears to be a smooth, elliptical-like structure, exhibiting a concentrated, bright core. This core gradually diffuses outwards into a more amorphous halo. There is also a fainter component that appears to be a disk-like structure, potentially indicative of spiral arms, but it is unclear. This feature is oriented at a sharp angle relative to the primary component. There appear to be slight distortions in the overall shape, which might indicate a minor gravitational interaction, but appears largely undisturbed. The color profile suggests a population of older stars, with a stronger presence in the central region and a less significant population in the outer disk. Star formation is expected to be low. 
