The galaxy presents as a generally smooth structure with an overall elliptical shape. The core region exhibits a high surface brightness, appearing bright white, suggesting a concentration of older stellar populations and minimal dust obscuration. A fainter, bluer halo surrounds the central region, indicating the presence of some younger stars and a degree of ongoing star formation. The galaxy exhibits a slight elongation, with the aspect ratio not far from round, but tending slightly toward an intermediate shape. There are no immediately obvious signs of major disturbances due to mergers or tidal interactions, although there is a possible minor disturbance detectable. There is a hint of a faint disk component.
