The galaxy presents a distinct spiral structure, with two prominent arms exhibiting a moderate winding. These arms emanate from a central bulge, which appears substantial. The color profile indicates a yellow-white hue toward the bulge, potentially suggesting an older stellar population and reduced star formation in this region. The spiral arms display a slightly bluer tone, possibly indicative of ongoing star formation activity. The overall disk appears tilted with the arms appearing elongated due to the angle of observation. There's a slight asymmetry to the disk, suggesting possible gravitational interaction or recent accretion events which may have led to disturbances within the galaxy.
