The galaxy presents a disk-like morphology, observed at an oblique angle. A central bulge is apparent, exhibiting a yellowish-orange hue, suggesting an older stellar population. Faint, diffuse spiral arms extend outwards from the bulge, exhibiting a bluer color profile relative to the central region, which suggests ongoing star formation. The overall structure displays some irregularities and asymmetry in the arms, possibly indicative of minor gravitational interactions or internal disturbances. Dust lanes are not clearly visible, but there appears to be some obscuration within the disk.
