The galaxy appears as a centrally concentrated object with a smooth, diffuse halo. The primary color is a pale blue-green, transitioning to a redder core, indicating a potential variation in stellar populations or dust content. The overall shape is elliptical, with the ratio of the major to minor axes suggesting a moderate degree of flattening. There is no apparent spiral arm structure or significant dust lanes visible. Faint, asymmetrical extensions or tidal features cannot be excluded based on the image quality, but they are not readily apparent. The galaxy seems relatively isolated, with no clear indication of ongoing major mergers or strong tidal interactions with other galaxies. The general morphology suggests a relatively evolved system, possibly an early-type spiral, or an elliptical galaxy.
