The galaxy presents a moderately inclined disk structure. Evident are spiral arms, though somewhat flocculent and not sharply defined. The central bulge appears small relative to the disk size, with a relatively low concentration of light towards the nucleus. The overall color index suggests a bluer disk indicative of ongoing star formation. Some morphological disturbance is apparent, possibly resulting from a minor interaction or internal dynamics. There is no clear bar structure visible. The galaxy is likely undergoing active star formation.