This galaxy presents as a flattened, disk-like structure, elongated along its major axis. The overall color is predominantly bluish, suggestive of active star formation. The central region appears slightly brighter, possibly indicating a higher stellar density or the presence of a bulge. There is some evidence of faint, spiral arm-like structures emanating from the central region, though these are not well-defined. The overall morphology could be described as a late-type spiral or an early-type barred spiral galaxy, seen at a relatively high inclination. The disk appears somewhat disturbed, hinting at possible past or ongoing interactions. There is little evidence of a prominent dust lane. The galaxy does not exhibit any obvious signs of a major merger, although the asymmetry and slight irregularities in the disk suggest minor disturbances. Overall, the galaxy appears to be a star-forming system of moderate size.
