The galaxy presents as a disk-shaped system, approximately 5.7 kiloparsecs in radius. There is a central bulge exhibiting a distinct reddish-orange hue, possibly indicative of an older stellar population or significant dust extinction. The disk component shows a more yellowish and muted color profile suggesting a mix of stellar ages. There may be some disturbance happening to the galaxy, because of its irregular edges. The galaxy is in between round and cigar shaped in morphology. Star formation rates are modest.
