The galaxy presents a largely smooth, elliptical morphology. It appears generally round in shape, with a slight deviation towards an intermediate ellipticity. No distinct spiral arm structures or a prominent central bar are discernible. The light distribution suggests a fairly uniform stellar population throughout the galaxy's visible extent, lacking significant color variations or distinct knots of star formation. There is no obvious evidence of a recent major merger event, though a minor disturbance may be present in the galaxy's outer regions, contributing to its slightly irregular shape. The galaxy's overall color is indicative of a relatively older stellar population, dominated by stars emitting in the redder portions of the spectrum. The galaxy shows moderate star formation activity. Overall, the galaxy appears to be a mature system, possibly an elliptical galaxy that has undergone some minor interactions.
