The galaxy presents as a spiral galaxy, observed at a significant inclination relative to our line of sight. The central bulge appears prominent, exhibiting a high degree of luminosity and a yellowish-white hue, potentially indicating an older stellar population. The disk structure is apparent, revealing spiral arm features that extend outwards from the central bulge.

The spiral arms appear somewhat flocculent and exhibit a blueish tint, suggesting ongoing star formation. There's a slight asymmetry observed within the disk, with one side exhibiting a slightly more defined spiral structure compared to the other. No obvious signs of major mergers or tidal disturbances are immediately apparent. The galaxy's overall morphology suggests a relatively undisturbed and evolved system.
