The observed galaxy presents as an edge-on spiral galaxy, exhibiting a disk-like morphology. A prominent bulge is observed, appearing rounded in shape. The disk itself appears relatively smooth, lacking significant indications of distinct spiral arm structures from this vantage point. There is a slight indication of a dust lane bisecting the galaxy along its major axis, suggesting the presence of interstellar medium obscuring light from the far side of the disk. The overall color appears to be yellow/orange, which potentially indicates an older stellar population and ongoing star formation. There are no obvious signs of major merger activity, though subtle disturbances or minor interactions cannot be entirely ruled out.