The galaxy presents a largely smooth, centrally concentrated morphology. It exhibits a generally elliptical shape with a high degree of roundness. There is a slight elongation, but it does not appear cigar-shaped. The galaxy's light distribution suggests a relatively uniform stellar population, with minimal discernible substructure in the image. There's a very slight suggestion of a disk, but the bulge dominates. The galaxy appears to be relatively isolated, showing no signs of major mergers, though a possible minor disturbance may be indicated by subtle irregularities in its overall shape. The galaxy displays a bluish-white hue.
