The observed galaxy appears to be a spiral galaxy, oriented approximately face-on relative to our line of sight. Two prominent spiral arms emanate from a central region with moderate bulge. The spiral arms are loosely wound, extending outwards from the nucleus. The arms display clumpy regions indicative of active star formation. The bluer hue of the spiral arms suggest a younger stellar population compared to the central region, which shows a slightly redder hue, possibly indicating an older stellar population. The central region appears relatively smooth. There is no obvious evidence of a strong bar structure. The general structure appears relatively undisturbed, suggesting no recent major merger events. The galaxy exhibits a disk-like structure. Overall, the galaxy presents as a well-formed spiral galaxy with ongoing star formation in its arms.
