The galaxy presents as a spiral type, displaying a discernible disk structure. Spiral arms are visible, though somewhat flocculent, with signs of ongoing star formation indicated by subtle blue hues interspersed throughout the arms. The central bulge appears relatively small compared to the overall disk size, showing a bright concentration. There is no strong indication of a central bar feature within the bulge region. The galaxy's disk does not appear to be oriented edge-on from our vantage point. No major merger events or tidal disturbances are readily apparent; however, there are hints of minor asymmetry or subtle irregularities in the outer regions of the disk, suggesting potential past interactions or minor disturbances. The galaxy presents an overall moderate inclination to our line of sight, allowing for a reasonable view of its spiral structure.
