The galaxy presents as an edge-on spiral system with a prominent, luminous bulge. The bulge exhibits a rounded morphology, showing a smooth distribution of light. The disk is clearly visible and appears to be relatively thin, exhibiting a notable degree of symmetry. There is no obvious sign of a strong bar structure. There is some clumpy structure along the galactic disk, which might be associated with star forming regions. The light is generally redder, which indicates an older stellar population or high dust obscuration, likely associated with ongoing star formation. Overall, the galaxy presents an undisturbed morphology.
