The galaxy appears to be a spiral galaxy viewed at a high inclination angle, close to edge-on. The central bulge is prominent and exhibits a smooth, concentrated light profile, appearing yellow-orange in color, which likely signifies an older stellar population. The galactic disk is visible, though not well-resolved, and appears elongated due to the viewing angle. There's some indication of faint, diffuse disk light extending beyond the bulge. Some irregularity and blueness in the disk indicates ongoing star formation. There's no obvious signs of major mergers or tidal disturbances in the system, suggesting a relatively isolated and undisturbed morphology.
