The galaxy presents as a relatively smooth, elliptical object. The light distribution is centrally concentrated with a gradual decrease in intensity moving outward from the core. No distinct spiral arms or significant dust lanes are readily apparent. The galaxy exhibits a rounded morphology, appearing nearly circular in shape. There is no obvious evidence of major mergers or significant tidal disturbances. Color gradients are subtle, with a yellowish core possibly indicative of an older stellar population and minimal ongoing star formation. The faint outer regions display a bluer hue suggesting the presence of some younger stars. Overall, the galaxy's appearance suggests a relatively evolved system with a smooth distribution of stars and minimal recent star formation activity.
