The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth with a concentrated central bulge. There is some evidence of a faint disk-like structure oriented along the major axis. Color gradients suggest a concentration of older stellar populations in the central region, appearing more reddish-orange, with hints of bluer, potentially younger stellar populations extending into the outer disk. There's no strong evidence of spiral arm structures or ongoing major mergers. Minor disturbances are not readily apparent, but subtle asymmetries in the light distribution can not be ruled out. The galaxy appears to be at a considerable distance, judging by its relatively small angular size.
