The galaxy presents as a highly inclined disk galaxy, likely viewed nearly edge-on. It exhibits a prominent central bulge with a moderate concentration of light. The bulge appears subtly boxy in shape. The disk component is elongated and relatively smooth in texture. The overall color is suggestive of an older stellar population, with a yellowish-orange hue dominating the central region. The outer regions of the disk exhibit a slightly bluer color, hinting at the presence of some younger stars or ongoing star formation. There is no obvious presence of strong spiral arm structure or dust lanes. The galaxy displays no distinct signs of recent major merger activity. The light distribution falls off gradually from the center, conforming loosely to a smooth Sersic profile.
