The galaxy presents as a luminous, elliptical or lenticular structure. It exhibits a centrally concentrated, smooth light distribution with a lack of defined spiral arms or a prominent disk component. The core region displays a high surface brightness, gradually decreasing towards the outer edges, suggesting a concentration of older stellar populations. A slight asymmetry is visible in its overall shape, possibly indicative of a minor interaction or past merger event, though no clear tidal features or strong disturbances are immediately apparent. The galaxy appears redder in color, suggesting an older stellar population and a low rate of ongoing star formation. The overall morphology points towards a galaxy that is relatively evolved and quiescent.
