The galaxy presents a generally smooth and featureless appearance. It is elliptical in shape, displaying a slight elongation, falling between a perfectly round and a more cigar-shaped morphology. The color gradient suggests a higher concentration of older stars toward the center, exhibiting a yellowish-red hue. The outer regions appear slightly bluer, hinting at the presence of a younger stellar population, although limited star formation activity is indicated throughout the galaxy. There is no discernible evidence of spiral arms or a prominent disk structure. No major merger events are apparent, though subtle disturbances might be occurring.
