The object appears to be a spiral galaxy, presenting a near face-on orientation relative to our line of sight. It exhibits two prominent spiral arms that originate near the central region, tightly wound, and extend outwards. These arms are well-defined and possess a somewhat fragmented appearance, suggesting regions of active star formation. The central bulge is relatively small but noticeable, presenting a yellowish hue that implies an older stellar population. A central bar structure appears to be present, oriented roughly vertically in this image. There seems to be a high rate of star formation.
