The galaxy presents as a centrally concentrated spheroid with a relatively smooth light distribution. The core exhibits a yellowish hue, suggesting an older stellar population. The light profile fades gradually from the center outwards, and the ellipticity of the galaxy is moderate, leaning toward a more circular shape rather than a highly elongated form. There is no clear evidence of spiral arm structure or significant dust lanes within the image resolution. Faint extensions hint at a broader halo, but distinct tidal features are not observed, indicating it does not appear to be undergoing any major merger events. There is some blue-ish light in the outer regions, perhaps indicative of some recent star formation. 
