The galaxy presents as a centrally concentrated, lenticular-like structure with a smooth, diffuse appearance. The core region exhibits a yellowish hue, suggestive of an older stellar population. Fainter, bluer light surrounds the core, indicating the presence of some younger stars or ongoing star formation, though at a seemingly low rate. The overall shape appears flattened, with a slight elongation visible. There's no clear evidence of spiral arms or a prominent disk structure. No major mergers or disturbances are visible, though there are some very faint hints of tidal tails.
