The galaxy appears to be a relatively luminous elliptical, exhibiting a smooth, centrally concentrated light profile. The core presents a yellowish-white hue, suggesting an older stellar population with a lower rate of active star formation, consistent with the observed color gradients. The galaxy displays a generally spheroidal morphology with a slight ellipticity; it's shape is generally round with a hint of elongation. No prominent dust lanes or spiral arm structures are discernible. Faint, diffuse light extends outwards from the core, gradually fading into the background, indicating a halo of older stars. There is no evidence of any major merger events or significant tidal disturbances. The overall appearance suggests a massive, evolved galaxy at a considerable distance.
