The galaxy presents as a lenticular or possibly an elliptical galaxy, viewed at a significant angle relative to its equatorial plane. It displays a smooth, elongated morphology with a high degree of ellipticity. The central bulge exhibits a pronounced concentration of light, appearing yellowish-orange, suggesting an older stellar population. Moving outward from the core, the galaxy exhibits a gradual decrease in surface brightness. Hints of bluer hues are present in the outer regions, possibly indicative of a small amount of ongoing star formation. There is no evidence of spiral arms or significant dust lanes within the visible portion of the galaxy. The overall structure suggests a relatively evolved system with a dominant spheroidal component. No signs of tidal disturbances or recent merger activity are apparent.
