The galaxy presents a roughly elliptical morphology, suggesting it might be an elliptical galaxy or a lenticular galaxy seen at a slight angle. It has a relatively smooth and homogenous appearance with little indication of spiral arms or significant dust lanes.

The color appears to be yellowish-orange, indicating a population of older stars and potentially a low rate of ongoing star formation. There is some variation in the intensity across the galactic body. The central region is distinctly brighter and more concentrated than the outer regions. The brightness gradient fades smoothly towards the edges. There is a faint suggestion of a possible tidal interaction or minor disturbance on one side, with an extended, slightly elongated, and fainter region emanating from the main body.
