The observed galaxy presents as a spiral galaxy with a relatively small bulge. Evident spiral arms emanate from a central region, exhibiting a somewhat flocculent structure. The arms show a degree of blueness, possibly indicating the presence of younger stellar populations. The bulge appears moderately bright and exhibits a yellowish or white hue. A hint of a bar-like structure seems present in the central region. The galaxy does not appear to be undergoing any major mergers, though the asymmetry may suggest some form of interaction or minor disturbance.
