The galaxy presents a primarily smooth morphology, with a high degree of central concentration. It exhibits a slightly elongated shape, leaning towards the 'in-between' roundness classification. There's no single clearly defined nucleus, but rather a gradual increase in luminosity towards the center of the galaxy. The color is predominantly yellow-white, with a hint of red on the periphery, possibly indicating some low-level star formation or an older stellar population in those regions. No spiral arms or distinct disk-like structures are apparent. There are possible signs of a minor disturbance on the outer edges, but no clear signs of a major merger event. The overall appearance suggests that the galaxy might be in a later stage of its evolution.
