The galaxy presents a moderately elliptical morphology. It appears to be a relatively smooth system, with a somewhat disturbed component. The central region exhibits a concentrated luminosity, suggesting a significant stellar population and potentially an active galactic nucleus or a supermassive black hole. A slight elongation is observed, though the overall shape is not highly flattened. The galaxy's color indices suggest the presence of both evolved stellar populations, contributing to the redder hues, and regions of ongoing star formation, indicated by the bluer tints, although this blue emission is less dominant. There is a slight indication of minor morphological disturbance, such as tidal tails or asymmetries, which might suggest a past or ongoing interaction with another galaxy. Overall, the galaxy appears to be a mature system, possibly undergoing minor evolutionary processes, such as accretion or minor mergers.
