The galaxy presents as a yellowish, elliptical-like structure. Its overall form appears relatively smooth, lacking prominent spiral arms or distinct features. The galaxy's core exhibits a high degree of concentration of light, suggesting a dense stellar population within the central region. There are no obvious signs of a major ongoing merger, though there may be signs of tidal disturbances or smaller companion objects in its halo. Faint wisps of material are visible in the halo of the galaxy, that indicate that the object might be undergoing or have recently undergone a merging event.
