The galaxy presents as a disk galaxy, viewed at a significant inclination. A central bulge is visible, exhibiting a yellowish-white hue, suggesting an older stellar population. From this vantage point, it appears to be a small bulge relative to the overall galaxy disk. The disk itself displays prominent spiral arm structure, tightly wound with active star formation regions visible as bluer patches within the arms. The galaxy's overall color gradient suggests ongoing star formation, with younger, bluer stars populating the spiral arms and an older, redder population concentrated in the bulge. A faint bar might be present across the nucleus. The overall morphology appears relatively undisturbed, without obvious signs of major merger events. The disk appears smooth and no tidal features are easily seen.
