The galaxy presents a clear disk-like structure, indicative of a spiral or lenticular morphology. A prominent central bulge is visible, exhibiting a concentrated brightness. Spiral arms appear to emanate from the central bulge region. These arms display a clumpy nature, potentially highlighting regions of active star formation within the galactic disk. The galaxy does not exhibit any signs of major interaction or disruption; it appears to be in a relatively undisturbed state. The bulge appears to be medium sized relative to the galaxy disk. There may be a bar going across the galaxy.