The galaxy presents as an elliptical morphology, with a relatively smooth light distribution. The central region exhibits a high concentration of light, appearing bright and slightly yellow/orange in color, suggesting a population of older stars. Moving outward from the core, the galaxy gradually fades, displaying a fainter, more diffuse halo. There is very little visible structure, such as spiral arms or dust lanes, contributing to its classification as likely elliptical or lenticular. The overall shape is close to circular but there is the slightest suggestion of some deviation. There's no clear indication of ongoing major mergers or significant tidal disturbances.
