This galaxy presents as a roughly elliptical structure with a concentrated central bulge that dominates the overall luminosity. The light distribution is relatively smooth, with a gradual decline in intensity from the core outwards. There are subtle indications of a disk-like component, however, the overall morphology suggests a galaxy undergoing transition from a disk-dominated system to a more spheroidal form. A faint, diffuse halo extends beyond the main body of the galaxy. It is difficult to resolve any significant spiral arm structure or dust lanes from this image, therefore the galaxy could be classified as an early-type spiral or a lenticular galaxy. Some minor disturbance can be seen in the periphery of the galaxy, hinting at tidal interactions with a nearby object in the past. Overall, the image suggests a galaxy with intermediate mass and moderate star formation.
