The galaxy presents as a diffuse, elliptical structure, exhibiting a smooth morphology. The central region displays a noticeable concentration of light, indicative of a galactic bulge. A gradual decrease in luminosity is observed from the core outwards. Coloration appears to be relatively uniform across the galaxy, with subtle variations suggesting differing stellar populations. The galaxy does not exhibit prominent spiral arms or significant dust lanes. Overall, the galaxy appears to be an early-type galaxy, likely an elliptical galaxy with a considerable stellar mass and a relatively low star formation rate. Slight indications of a minor disturbance can be seen in the asymmetry of the halo. The overall shape of the galaxy is in between a round and cigar shape.
