The observed galaxy presents a flattened, disk-like morphology with a bright, concentrated central bulge. The bulge appears yellowish-orange, suggesting an older stellar population and/or the presence of dust obscuration. Extending from the central region is a fainter, bluer disk.

The disk exhibits structural irregularities. Faint, patchy features are observed. The edges of the disk appear somewhat diffuse and uneven, hinting at possible tidal interactions or disturbances. The orientation is nearly edge-on, allowing for an estimation of the galaxy's flattening.
