The observed galaxy presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Emanating from the central bulge are spiral arms, exhibiting a blue tint, indicative of ongoing star formation. These arms show a loose winding pattern. A slight asymmetry can be observed in the arm structure, potentially indicative of a minor gravitational interaction or recent merger event. The disk appears relatively smooth, with subtle dust lane features. The overall light distribution suggests a Sersic profile, transitioning from the bright central bulge to the fainter outer disk.
