The observed galaxy presents as a highly inclined, likely edge-on, disk galaxy. A prominent central bulge is apparent, displaying a concentrated, yellowish-orange hue, suggestive of an older stellar population dominating the galactic core. The disk component exhibits a bluer tinge compared to the bulge, potentially indicative of ongoing star formation within the galactic plane. The dust lane obscuring the midplane is subtle, and the bulge appears smoothly integrated into the surrounding galactic disk. There is no clear indication of a strong bar structure or any signs of major mergers. The overall morphology suggests a relatively undisturbed system.
