The galaxy presents as a spiral, observed at a significant inclination, approaching edge-on. A prominent central bulge is observed, elongated along the major axis of the disk. Spiral arms appear tightly wound around the bulge. There is evidence of a strong bar structure spanning the bulge region. The overall color profile suggests active star formation, with a bluer hue detected along the disk and a redder hue more concentrated in the bulge. No major signs of recent or ongoing major mergers are apparent, but there is some possibility of minor disturbances as the galaxy's shape is not perfectly symmetrical. The arms feature patches of light indicative of the presence of HII regions. The galaxy is relatively massive and actively forming stars.
