The galaxy presents an overall elliptical morphology. The central region exhibits a pronounced bulge with a yellowish-orange hue, suggesting an older stellar population. Progressing outward, the galaxy shows a transition into a more flattened disk-like structure. This region displays a greenish tint, possibly indicating the presence of younger stars or ionized gas, though any distinct spiral arm structure is not readily apparent. The galaxy's shape appears elongated, leaning towards a cigar-like form. There's no noticeable sign of major mergers or significant tidal disturbances in the surrounding regions, though subtle irregularities hint at possible minor interactions.
