The galaxy presents a generally smooth, elliptical appearance with a relatively high degree of central concentration. It has a flattened, cigar-like shape. There is evidence of potential minor disturbances, with some asymmetries that hint at past or ongoing interactions, although the object is not undergoing a major merger. The galaxy exhibits a broad color profile suggesting a moderately quiescent stellar population. The half-light radius of the galaxy is relatively compact. The light distribution suggests a more evolved system with a lower rate of star formation.
