The galaxy presents as a somewhat amorphous and indistinct object. Its morphology appears to be largely smooth, with a slightly elongated shape. A central concentration of light is present, giving the impression of a bulge. Patches of reddish hues are scattered within the galaxy's structure, perhaps indicative of areas of older stellar populations or dust obscuration. A faint disk-like structure may be present, though it is difficult to discern due to the galaxy's indistinct form. There are also faint blue regions that may be present on the galaxy. The overall color suggests a mix of stellar populations, likely with older stars dominating. There is also an irregular structure that may be caused by a minor merger. The presence of these features leads to the conclusion that this galaxy is an intermediate mass system with moderate ongoing star formation and is actively merging with a smaller system. 
