This galaxy appears to be a spiral type, viewed at an oblique angle. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. Faint, tightly wound spiral arms extend from the bulge, exhibiting a bluish tint, indicative of ongoing star formation. There are indications of two distinct, possibly tightly-wound, spiral arms. The disk appears relatively smooth and undisturbed. The orientation gives the appearance of a moderate thickness. The colour of the disk appears to subtly shift from blue near the edges to yellow closer to the bulge. There is no obvious tidal tail or distortion, and no evidence of a major merger event.
