The galaxy presents as an elongated, edge-on spiral. It is characterized by a prominent central bulge that appears relatively smooth and concentrated, exhibiting a yellowish hue, possibly indicating an older stellar population. The galactic disk is visible as a fainter, bluer extension along the major axis, suggesting the presence of ongoing star formation. A dust lane is suspected to be present running along the major axis of the galaxy due to the slight color difference observed in the disk region. The overall structure is relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. There may be a minor disturbance in the disk.
