The galaxy appears as an elliptical-like structure, exhibiting a predominantly smooth morphology with a concentrated central bulge. The light distribution suggests a relatively uniform stellar population across the main body, with a noticeable color gradient. The core region shows a yellowish hue indicative of older stars and lower star formation activity, while there are slight hints of bluer regions in the galaxy's halo, potentially regions with ongoing star formation, though limited. The shape is largely in between round and cigar shaped. There are some minor disturbances that suggest interactions or past mergers. There is no clear evidence of spiral arms or prominent dust lanes.