The galaxy presents as a predominantly smooth, elliptical-like structure with a concentrated, bright central bulge. Its overall shape is generally round. Faint, diffuse features extend outward from the central region. There is no distinct spiral arm structure visible; however, some minor disturbances or irregularities may be present in the outer regions, potentially indicative of interactions or minor mergers, but most likely not. The colour profile suggests a relatively evolved stellar population with a higher concentration of older, redder stars in the central region and an overall yellowish hue. The galaxy doesn't appear to be currently undergoing a major merging event.
