The galaxy presents as a largely smooth, elliptical form. Its core exhibits a bright, concentrated intensity, suggesting a significant stellar density. The overall color appears reddish, possibly indicative of an older stellar population and lower rates of current star formation. There is a subtle color gradient extending outwards from the core to its periphery, which could reflect differences in metallicity or stellar population. The object appears relatively isolated, exhibiting no obvious signs of ongoing major mergers, though a minor disturbance or interaction cannot be completely ruled out based on visual inspection alone. The morphology tends toward a spheroidal shape, as opposed to a flattened disk-like structure.
