The galaxy presents a largely smooth and centrally concentrated morphology, indicative of an elliptical or lenticular type. There appears to be minimal evidence of spiral arms or significant disk structure. The color profile suggests a dominance of older stellar populations, with a yellowish-red hue in the central region. There is a slight asymmetry in the shape, with a marginal deviation from perfect roundness. The galaxy may have experienced or be undergoing a minor interaction, though it has no major signs of disturbance. It does not seem to be undergoing a major merging event. The projected size appears relatively compact.
