The galaxy appears to be an edge-on spiral galaxy. A distinct dust lane bisects the galaxy's disk, absorbing a significant portion of the light from the bulge. The central bulge region exhibits a yellowish hue, possibly indicating an older stellar population. Surrounding the bulge, the disk appears bluer, suggesting ongoing star formation. There is a slight indication of possible asymmetries within the disk, but it is difficult to distinguish whether these are actual tidal features or simply due to light obstruction from the galaxy's dust lane. Overall, this appears to be an undisturbed disk galaxy undergoing active star formation.
