The galaxy presents a morphology consistent with a spiral galaxy, viewed at an oblique angle. The central bulge is prominent and exhibits a concentrated, bright luminosity profile, suggesting an older stellar population. The disk shows well-defined spiral arms that are wound moderately tightly around the bulge. These arms display a clumpy structure, indicating active star formation regions. Two primary arms are discernible. The overall color of the disk appears bluish, indicative of ongoing star formation, though the central regions exhibit a more yellowish hue. There is a possible bar structure spanning across the central bulge, extending into the inner disk region. No significant signs of major tidal disturbances or interactions with other galaxies are immediately obvious. The galaxy seems to be relatively isolated and unperturbed.
