The galaxy presents as an edge-on spiral. It exhibits a prominent, somewhat elongated bulge that appears to be relatively smooth and rounded. The disk is clearly visible, showing a distinct flattening and a slightly warped appearance. The color distribution suggests an older stellar population within the bulge, indicated by its redder hue. The disk shows a more complex color gradient. There is no clear evidence of significant ongoing star formation. The overall morphology appears relatively undisturbed, with no strong indications of a major merger event, although there may be some signs of a minor disturbance.
