The galaxy presents as a relatively small, moderately bright object with a lenticular or possibly an elliptical morphology. The main body of the galaxy appears diffuse, exhibiting a smooth light distribution with a centrally concentrated bulge that is slightly elongated along the major axis. Faint hints of a disk-like structure can be discerned, although the image resolution is limited.

The galaxy's color gradient suggests an older stellar population, as indicated by its yellow-white hue. Star formation appears to be low. There are subtle indications of a minor disturbance in the galaxy's structure, possibly due to a past interaction with another galaxy. The overall structure is neither perfectly smooth nor entirely disk-dominated, placing it somewhere on the transitional scale between elliptical and spiral types.
