The galaxy presents as an elliptical or lenticular system with a smooth, generally featureless morphology. Its color appears predominantly yellow/orange, suggestive of an older stellar population with minimal ongoing star formation. The central region exhibits a brighter concentration of light, indicating a nucleus, possibly harboring a supermassive black hole. The light distribution gradually diminishes outwards from the core, lacking any distinct spiral arm structures or prominent dust lanes. There is a slight indication of a minor disturbance in the galaxy's morphology, which may be caused by tidal interactions or a minor merger. It has a slightly elongated shape, appearing between round and cigar-shaped.
