The galaxy presents a largely smooth and rounded morphology, with a high degree of central concentration. It appears as a relatively compact object, potentially an elliptical galaxy. The galaxy's color profile seems to indicate a population of older stars, with minimal ongoing star formation visually apparent, giving it a relatively redder appearance. There is no obvious spiral arm structure, dust lanes or significant distortions, suggestive of a system that is dynamically settled, with no major mergers currently in progress. There is a possible minor disturbance or interaction with a small, nearby object. The overall structure suggests a evolved galaxy.
