The galaxy presents as a spiral type, viewed at an oblique angle to our line of sight. This orientation allows for discernment of the disk structure. The galaxy exhibits prominent, well-defined spiral arms. The winding of these arms appears to be of medium tightness. The galaxy's disk shows a mottled texture, suggestive of ongoing star formation regions. A central bulge is evident, with an intermediate relative size compared to the disk. The overall color of the galaxy appears blueish, indicative of a relatively young stellar population. There is no strong visual evidence of a prominent bar structure. The galaxy appears relatively undisturbed, without major signs of mergers or tidal interactions. The light is more concentrated at the center, but appears to spread toward the edges of the disk.
