The galaxy presents as a relatively smooth, centrally concentrated system. It appears to be an early-type galaxy, possibly elliptical or lenticular, characterized by a generally spheroidal shape. The light distribution is not perfectly circular, displaying a slight deviation towards an elongated form. There appears to be some tidal disturbances within the galaxy, suggesting possible recent interactions with another galaxy. The light from the galaxy shows a smooth color gradient from the core to the outer region, suggestive of an older stellar population with some ongoing star formation. There is a suggestion of weak spiral arm structures within the galaxy.

The galaxy appears to be a merging system.
