The galaxy presents as a relatively bright, isolated object exhibiting a moderately concentrated morphology. Its overall form is lenticular, with a predominantly smooth light distribution across the main body. There is little evidence of spiral arm structure. Subtle color gradients suggest older stellar populations concentrated toward the center. The galaxy exhibits modest ongoing star formation, inferred from the relatively bluer color. No major disturbances or signs of a recent merger are apparent in its structure. The shape appears close to round, with a moderate ellipticity. The galaxy seems to be a single entity.
