This galaxy presents a predominantly smooth morphology, appearing elliptical in shape. It displays a noticeable central bulge that gradually diffuses into the surrounding galactic halo. The color profile is relatively uniform, with a slight blue tint, indicating a moderate level of ongoing star formation. There is no clear evidence of distinct spiral arms or a prominent disk structure. The overall impression is that of a mature galaxy, possibly in the process of transitioning to a more quiescent state. Subtle disturbances in the outer regions suggest a potential history of minor gravitational interactions, although no major merger events are immediately apparent.
