The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears to be elliptical or lenticular, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a bright, concentrated core, possibly indicating the presence of an active galactic nucleus or a dense stellar population in the galactic center. The light appears to be dominated by older stellar populations. There may be some dust and gas present, given the small amount of color observed. The overall structure suggests a galaxy that has undergone significant evolution. There is a slight hint of disturbance.
