The galaxy appears to be a relatively large spiral galaxy seen at an intermediate inclination. The central bulge dominates the morphology, displaying a smooth, concentrated light profile with a yellowish hue, suggesting an older stellar population. Fainter, bluer spiral arms extend from the bulge, though they are not well-defined and appear somewhat diffuse. The galaxy is generally elongated, deviating from a perfectly circular shape. There is very little evidence of strong ongoing star formation. Overall, the galaxy presents a fairly relaxed morphology.
