The galaxy presents as an elongated, disk-like structure seen edge-on. A prominent central bulge is observed, appearing bright and yellowish, suggesting a concentration of older stellar populations. The disk component exhibits a gradient of color, with the regions closer to the bulge appearing more yellow and those farther away displaying a bluer hue. This implies the presence of younger, hotter stars in the outer regions. The disk appears somewhat disturbed. Patches and flocculent regions are visible in the disk, possibly indicating areas of active star formation. There is no clear evidence of a major merger or significant tidal disruption. 
