The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that appears yellowish-white in color, potentially indicating an older stellar population. The galaxy is somewhat elongated, with a cigar-like shape, and the outer regions display a subtle fading in luminosity, transitioning into a diffuse halo. No distinct spiral arm structure or significant dust lanes are apparent. There are no obvious signs of major disturbances or mergers, suggesting a system currently in a relatively quiescent state. Faint blue tinges are subtly present which could indicate low levels of on-going star formation. Overall, the galaxy appears to be a relatively evolved system.
