The galaxy presents a flattened, disk-like morphology but also a significant central bulge. The bulge appears relatively smooth and featureless. The disk component exhibits some visible structure, potentially indicating spiral arms, however these are not particularly well-defined. The overall color of the galaxy appears somewhat redder, suggesting a population of older stars and less ongoing star formation. There may be some minor disturbances within the disk, which could imply recent interaction or merger events. The general shape seems more in between round and cigar shaped, leaning towards a elongated appearance. There is no clear presence of a major ongoing merger, although the possibility of minor interactions or past mergers impacting the morphology cannot be ruled out. The overall appearance suggests an intermediate disk galaxy, with indications of a transition towards a more lenticular, smooth morphology.
