The galaxy presents as a spiral type, exhibiting a prominent, moderately sized central bulge. Spiral arms are clearly visible, displaying a well-defined structure, with primarily two arms emanating from the central region. The winding of the spiral arms appears to be of medium tightness.

The galaxy's disk is not edge-on, allowing for clear observation of the spiral structure. There's a strong possibility of a bar structure within the central region, though not exceedingly prominent. The arms themselves show hints of flocculent structures and some apparent disturbances, suggesting potential minor gravitational interactions, although a major merging event does not seem to be occurring. The galaxy is slightly blue overall, suggesting an ongoing stellar formation.
