The galaxy presents as a spiral type, with a clearly defined disk structure. The spiral arms are prominent and numerous, tracing a relatively tight winding pattern. The color profile suggests ongoing star formation within these arms, indicated by the bluer hues interspersed with regions of more mature stellar populations showing as redder areas. A bar feature is discernible crossing the central region. The bulge appears to be of moderate size relative to the disk. There is no obvious sign of major disturbance.
