This galaxy presents as an edge-on spiral. There is a prominent central bulge with an elliptical shape that transitions smoothly into the disk. Dust lanes are visible along the plane of the disk, obscuring some of the light from the bulge. The color distribution across the galaxy shows a redder hue in the central bulge, suggestive of an older stellar population. The disk appears bluer, indicating regions of ongoing star formation. The galaxy does not display any obvious signs of recent major merger activity, although there might be minor disturbances or asymmetries within the disk that cannot be clearly distinguished due to the angle of observation. The galaxy appears relatively undisturbed, without any significant tidal tails or distortions. Overall, it seems to be a relatively normal, quiescent spiral galaxy viewed edge-on.