The galaxy presents as an elongated, disk-shaped structure oriented approximately vertically in the image. A central bulge is visible, appearing brighter and more concentrated than the surrounding disk. The disk itself exhibits a mottled texture with diffuse, asymmetric spiral arm features that are not clearly defined, suggesting they are either tightly wound, disrupted or simply too faint. These arms present a bluer hue, suggestive of recent star formation. There is no single dominant arm. The overall color of the galaxy leans towards a bluer tint, contrasting with the yellowish hue of the central bulge, which implies a possible presence of an older stellar population. There may be some minor signs of gravitational disturbance or interaction, given the asymmetry and diffuse nature of the spiral arms, although these could also be intrinsic features of the galaxy's morphology.
