This galaxy exhibits a pronounced disk morphology with a notable central bulge. The disk is not viewed perfectly edge-on, but at an angle with a high degree of inclination. The bulge appears to be a significant component of the galaxy's overall structure, extending substantially into the disk region. Faint spiral arm structures are visible, with a tightly wound appearance. Two prominent arms are observed. Indications of a bar structure bisecting the central bulge, but it is more difficult to fully resolve. The galaxy's color profile shows a central concentration of yellowish light, transitioning to a more bluish hue in the outer disk regions, potentially indicating differing stellar populations. The overall structure suggests that this galaxy could have experienced some kind of merging event. The overall structure is indicative of a classic spiral morphology. 
