The galaxy presents as a spiral type with a prominent disk structure. Spiral arms are distinctly visible, exhibiting a somewhat flocculent morphology. The central bulge appears relatively small and compact, with a bright, concentrated core. There is evidence of active star formation, indicated by the presence of blue-ish regions along the spiral arms and near the outer edges of the disk, showing active star formation. Dust lanes are subtly visible, obscuring some of the light from the disk, and it appears to be a relatively isolated galaxy, showing no major signs of interaction or merging, but some minor disturbance may be present. Overall, the galaxy appears to be of moderate size and luminosity for its type.
