The observed galaxy presents as an edge-on spiral. The disk appears elongated with a relatively smooth, bright central bulge that fades into the disk. There's a slight indication of dust lane absorption along the central plane, lending credence to its classification. The color gradient shows a slightly bluer hue towards the outer regions of the disk, indicative of ongoing star formation, which is consistent with the estimated star formation rate. No prominent tidal features or major disturbances are discernible, though there may be a very small companion or background galaxy. The galaxy does not appear to be in a major merger state.
