The galaxy presents as a spiral with a prominent disk structure. A central bulge is visible, appearing moderately sized. Two spiral arms are clearly defined, exhibiting a medium winding pattern around the central bulge. There appears to be no strong bar feature. Evidence of ongoing star formation is present within the spiral arms. Overall, the galaxy displays a normal spiral morphology with a slight inclination, and a relatively high degree of symmetry. Some minor disturbances or irregularities are also observed, indicating possible recent interaction or internal activity. The galaxy appears to be relatively isolated.
