The galaxy presents as a spiral type, viewed nearly face-on. Prominent spiral arms extend from the central bulge, exhibiting a fairly tight winding pattern. The arms display clumpy structures that suggest active star formation regions. A bar-like feature appears to traverse the central region, potentially influencing the spiral arm structure. The central bulge appears moderately sized and exhibits a yellowish hue, indicative of an older stellar population. There is no apparent presence of any major ongoing merging event, but there are possibly some minor disturbances. Overall, this galaxy appears to be a fairly massive, star-forming spiral galaxy at moderate redshift.
