The galaxy presents as a spiral galaxy with a prominent disk structure. Spiral arms are visible, tightly wound around a moderately sized central bulge. There is no evidence of a strong bar structure. The bulge appears yellowish, suggesting an older stellar population. The spiral arms display a bluer hue, indicative of ongoing star formation. The arm definition varies; some segments appear more clearly defined than others. No significant tidal disturbances or signs of major merger events are readily apparent, although minor perturbations or asymmetries might be present upon closer inspection. The overall impression is that of a relatively isolated, well-formed spiral galaxy. The arm count is hard to distinguish in the outer arms due to noise and the angle of the galaxy relative to our viewpoint. The central region is somewhat saturated, making detailed analysis of the bulge difficult.
