The galaxy appears as a prominent, reddish-orange elliptical or lenticular structure, exhibiting a relatively smooth morphology. There is a concentrated central bulge with a somewhat diffuse halo. There seems to be a possibility of minor disturbances in its structure, suggesting potential interactions or previous merger events. The galaxy's overall shape is approximately round, but has a subtle elongation. The red color suggests the presence of an older stellar population and relatively low levels of current star formation.