The galaxy presents as a disk galaxy observed nearly edge-on. A prominent central bulge is apparent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk appears relatively smooth and flattened with a faint, blueish tinge to the edges. There is no apparent dust lane visible, nor distinct spiral arm structure. The overall morphology indicates a galaxy with a relatively high stellar mass and low ongoing star formation rate. The system does not show any obvious signs of interaction or recent merger activity.
