The galaxy presents as a relatively small, elliptical object with a high degree of smoothness. The central region appears as a concentrated, bright core, indicative of a significant stellar population and potentially a supermassive black hole. Moving outward from the core, the luminosity gradually decreases, forming a diffuse halo. The overall color is somewhat reddish, possibly due to an older stellar population with lower star formation rate. There is a slight flattening of the galaxy along one axis, suggesting it is not perfectly spherical but rather an oblate spheroid. There is also a slightly brighter spot on one side of the halo. There are no apparent spiral arms or dust lanes. The galaxy appears largely undisturbed, without signs of major recent mergers or tidal interactions.
