The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, spheroidal morphology with no discernible spiral arm structure. The light distribution is concentrated towards the center, fading gradually towards the edges. There is a potential for an ongoing or recent merger, indicated by the somewhat irregular overall shape and the presence of possible tidal features or disturbances in the outer regions. The galaxy's color suggests a dominant population of older stars. Star formation appears to be relatively low.
