The galaxy presents as a face-on spiral structure. Predominantly blue-shifted light emanates from its spiral arms suggesting active star formation, while the central bulge exhibits a yellower hue, potentially indicative of an older stellar population. The spiral arms appear tightly wound. A weak bar structure is suspected traversing the central region. There is no evidence of a substantial bulge component, nor any prominent signs of ongoing major merger activity. Evident is a slightly irregular morphology, possibly due to minor gravitational interactions or internal processes affecting the disk structure. The galaxy exhibits a generally smooth appearance interspersed with patches of greater intensity suggesting uneven star formation.
