The galaxy presents a lenticular morphology. Its overall shape is elliptical but exhibits some disk-like features. The light distribution appears relatively smooth, suggesting an older stellar population. The galaxy is viewed at a moderate inclination angle, allowing a partial view of the disk. There is no obvious presence of spiral arms. Faint disk-like features are visible, hinting at some remaining rotational dynamics. There is no distinct central bulge, although some central concentration of light is noted. No tidal tails or other signs of ongoing or recent major merger events are apparent. The galaxy appears isolated.
