The galaxy presents as a somewhat flocculent spiral with moderate central bulge prominence. The arms are not tightly wound; they appear relatively open and slightly patchy in structure. There is evidence of ongoing star formation, visible in the blue-tinged regions within the spiral arms. The central bulge exhibits a more yellow/orange hue, suggesting an older stellar population. The overall light distribution is moderately smooth but contains noticeable irregularities and disturbances, and there are signs of potential minor interaction or tidal features, though they are not strongly pronounced. The shape is elliptical in projection. 
