The observed galaxy presents as a spiral galaxy, exhibiting a prominent disk structure. The central bulge is clearly defined and of moderate size relative to the overall galaxy dimensions. Within the disk, two dominant spiral arms are discernible, with a relatively tightly wound morphology. A strong bar structure appears to be present across the central region of the galaxy. Visual inspection suggests that the galaxy is not undergoing any significant merger activity, although there is some suggestion of a slight disturbance in the overall structure.
