The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge dominates the core region, exhibiting a yellowish-orange hue suggestive of an older stellar population. The disk appears relatively smooth, lacking significant resolved star-forming regions or prominent spiral arms. Faint blueish regions extend outwards from the central bulge along the plane of the disk, indicating the presence of some younger, bluer stars, possibly areas of recent, low-level star formation. There is no obvious signs of recent major merger activity, although there is the possibility of a minor tidal disturbance. The overall morphology suggests a galaxy transitioning towards a more quiescent state, with a declining star formation rate.
