The galaxy appears to be a spiral galaxy viewed almost perfectly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge region. The bulge exhibits a generally rounded morphology with a diffuse appearance; there is no distinct nucleus discernible. The disk component is visible as a flattened structure extending outwards from the bulge on either side, with a noticeable fading in brightness towards the outer edges. The disk appears relatively smooth and featureless, lacking readily identifiable spiral arm structures or prominent star-forming regions. Faint extensions emanating from the main body can be observed, appearing asymmetrical in nature. The galaxy exhibits a relatively smooth color gradient, shifting from a slightly redder hue towards the central bulge to a somewhat bluer tinge in the outer disk regions. Overall, the galaxy presents a well-defined, elongated shape characteristic of an edge-on spiral galaxy with a considerable dust component. The lack of significant irregularities suggests it is not undergoing any major ongoing merger events, though some minor disturbance cannot be ruled out.
