The galaxy appears to be a spiral type, viewed at an oblique angle. The central bulge is prominent and exhibits a smooth, concentrated light profile, suggestive of an older stellar population. The disk component is evident, displaying a distinct blue hue, possibly indicative of ongoing star formation within its spiral arms. The arms themselves seem tightly wound around the central bulge, and there appears to be two. Faint disturbances or asymmetries are observed in the outer regions of the disk, potentially indicating minor interactions or past merger events. There may be a bar. The overall structure suggests a galaxy with a moderate to large bulge and active star formation within its spiral arms.
