The galaxy presents as a spiral, observed at a high inclination with respect to our line of sight. The central bulge appears elongated, suggesting the presence of a bar structure. The bulge exhibits a yellowish hue indicative of an older stellar population. The disk is visible but somewhat faint, with a bluish tint that likely corresponds to ongoing star formation. The spiral arms are not sharply defined, and display a flocculent morphology. Overall, the galaxy exhibits characteristics of a disk galaxy, undergoing some star formation. There is no obvious indication of any major tidal disturbances or merging events.
