The galaxy presents as a spiral, viewed at an oblique angle, but not quite edge-on. The central bulge appears moderately prominent and luminous, with a diffuse glow. There is evidence of discernible spiral arms that are not tightly wound, exhibiting a flocculent structure. Patches of bluer light are interspersed within the arms, possibly indicating regions of more recent or ongoing star formation. The disk appears relatively extended, with a slight asymmetry in the distribution of light, potentially indicative of a minor gravitational interaction or internal disturbance. No strong bar feature is readily apparent, although a weak linear structure may be present in the central region. The overall color profile suggests a mix of stellar populations, with the bluer regions associated with younger stars and the more yellow/red colors potentially indicative of older stellar populations.
