The galaxy exhibits a distinct spiral morphology, with well-defined, though somewhat flocculent, arm structures extending from a central bulge region. The arms appear relatively open, suggestive of grand design spiral characteristics. The color profile indicates a bluer hue concentrated within the spiral arms, which likely corresponds to regions of active star formation. The central bulge displays a more uniform color profile. Overall, the system presents a disk-dominated appearance. Irregularities are visible within the disk which may be merger activity or interactions with smaller satellite galaxies. There does not seem to be a strong bar structure.
