The galaxy presents as a likely spiral type, though the relatively low resolution somewhat obscures detailed morphological features. A central bulge region is evident, exhibiting a yellowish-orange hue, which may indicate an older stellar population with fewer young, massive stars. Fainter, bluish-greenish patches are observed in what appear to be extended arms or a disk structure surrounding the bulge. These likely indicate regions of ongoing star formation where hot, young stars ionize surrounding gas. There appears to be some degree of disruption visible in the galaxy's structure. There is a neighboring galaxy on the right which is also a bluish-green color. It is possible this galaxy is in the process of a minor merger or a close gravitational interaction which would explain the irregular shape and disrupted spiral arms.
