The galaxy presents a disk-like morphology, viewed at a slight inclination. It exhibits prominent spiral arm structures. There is evidence of a central bulge. The color gradient indicates a potential distribution of stellar populations, with a bluer hue in the outer regions possibly indicating ongoing star formation and redder hues towards the center suggestive of older stellar populations. There is no obvious sign of a major merger event, although minor disturbances cannot be ruled out. A strong bar seems present within the bulge. The overall appearance suggests a galaxy with a substantial disk component and active star formation, particularly within its spiral arms.
