The galaxy presents a distinctly disk-like morphology, viewed at an angle that is not quite edge-on. The central bulge is moderately prominent, exhibiting a soft, diffuse glow that graduates into the surrounding disk. Spiral arm structures are clearly discernible, exhibiting a relatively open winding pattern as they extend from the central region. There may be two dominant spiral arms. The disk component shows areas of bright and less bright spots. Overall, the galaxy appears largely undisturbed, with no obvious signs of ongoing major mergers, although subtle disturbances in the disk's symmetry could indicate minor gravitational interactions. The overall color suggests a relatively active star formation rate.