The galaxy presents an edge-on morphology, with a prominent, relatively bright central bulge. The bulge exhibits a yellowish-orange hue, suggestive of an older stellar population with a lower rate of on-going star formation. A disk component is clearly visible, extending outwards from the bulge along a horizontal axis. This disk component exhibits a bluer color, particularly towards the edges. The bluer color of the disk hints at regions with active star formation and a younger stellar population. The galaxy displays a relatively smooth overall appearance. However, a slight asymmetry or warping can be perceived at the extreme ends of the disc, warranting further investigation to determine if this is the result of a minor interaction with another galaxy.
