The galaxy presents as a spiral type, exhibiting a discernible disk structure that is oriented face-on relative to our line of sight. The spiral arms are prominent, displaying a generally moderate winding pattern. Two main spiral arms are clearly visible, emanating from the central region.

A bulge component is observed, appearing to be of moderate size relative to the overall disk. There is a suggestion of a bar-like structure within the central region, though it does not appear to be a particularly strong or well-defined feature.

No obvious signs of major mergers or significant disturbances are evident in the galaxy's morphology. The overall appearance is relatively undisturbed, suggesting a quiescent evolutionary state. The galaxy appears to be relatively smooth in texture, with no obvious signs of starburst activity.
