This galaxy presents a smooth, elliptical morphology. The central bulge is dominant, appearing nearly spherical. A faint, diffuse halo surrounds the core, gradually fading into the background sky. There is no evidence of spiral arm structure or significant dust lanes. The galaxy displays a notable color gradient, with the central region exhibiting a more reddish-yellow hue, suggesting an older stellar population. Moving outward, the color appears to become slightly bluer, potentially indicating the presence of younger stars in the outer regions, although this is not pronounced. The lack of any obvious disturbances or tidal features suggests the absence of recent major merger events.
