The galaxy presents as a somewhat elongated, disk-like structure. A central bulge region is visible and appears to be composed of older stellar populations, exhibiting a yellowish hue. The disk shows hints of blue regions, suggesting ongoing star formation activity. There are features indicating possible disturbances and asymmetries in the galaxy's structure, and a large amount of light from a possible merger. The main component of the galaxy is largely smooth. The isophotes are generally elliptical in shape, leaning toward a intermediate shape between round and cigar shaped.
