The galaxy presents as a relatively smooth, elongated structure. Its overall shape is reminiscent of a cigar, indicating it is likely an elliptical galaxy. The central region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. The outer regions of the galaxy appear fainter and somewhat redder, possibly indicating the presence of more evolved stars or dust obscuration. There is no distinct evidence of spiral arms or active star formation. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers, although a slight disturbance is possible given some slight asymmetry in the extended halo.
