The galaxy presents as a centrally concentrated, ellipsoidal structure. The core region displays a pronounced luminosity, appearing almost uniformly bright with a yellowish hue. Moving outwards from the core, the light gradually diminishes into a diffuse halo, elongated along one axis, giving the galaxy an overall cigar-like shape. There is little to no resolved substructure visible in this image; the galaxy appears largely smooth, with no prominent spiral arms or dust lanes discernible. A small amount of blue light is visible on the edges. No signs of major mergers or tidal disturbances are immediately obvious from the observed morphology. It seems to be an isolated object.
