The galaxy presents a clear spiral morphology. It is not observed edge-on; it appears to be face-on or at a slight inclination. A central bulge is present, appearing moderately sized. The spiral arms are well-defined, exhibiting a relatively medium winding pattern. Two distinct arms appear to dominate the structure. No strong bar is apparent within the central region, although there is some indication of a weaker bar structure. The overall appearance suggests ongoing star formation, particularly within the spiral arms, based on the distribution of light. No major merger event is immediately obvious, though there is some asymmetry in the outer regions of the galaxy, hinting at a possible minor interaction or internal disturbance. The galaxy's color indices imply it hosts both older stellar populations within the bulge and younger, bluer stars concentrated along the spiral arms.
