The galaxy presents as an elliptical or lenticular system, with a smooth, centrally concentrated light profile. It appears largely featureless, lacking prominent spiral arms or significant dust lanes. The core region exhibits high luminosity, suggesting a dense stellar population or active galactic nucleus, though the resolution is insufficient to confirm the presence of the latter. The light gradually decreases outwards from the center of the galaxy. Overall, the galaxy appears to be in a relatively quiescent state, with limited ongoing star formation. Its shape is noticeably elongated but not extremely so. There is no obvious sign of any recent or ongoing merging activity.
