The galaxy presents as a singular, luminous object with a centrally concentrated morphology. The light profile appears relatively smooth, suggesting a dominant spheroid component. There is an extension of light outward from this central bulge, and appears to have a somewhat tidal shaped appearance. The overall color of the galaxy appears redder, implying an older stellar population. Evident is a possible core merging signature, suggesting the possibility of the galaxy being composed of two distinct centers or being actively involved in a merger event. This object is most likely an elliptical galaxy.
