The galaxy appears to be a spiral galaxy, viewed at a slight angle. It exhibits a prominent central bulge with a yellowish hue, suggesting an older stellar population. Fainter, bluer spiral arms extend outwards from the bulge, indicating ongoing star formation. The arms appear tightly wound around the central bulge. A bar structure is visible in the center of the galaxy. The overall shape suggests a moderately massive galaxy with an active star formation rate. There are no obvious signs of a major merger or significant tidal disruption.
