The galaxy presents as a relatively smooth, elliptical object, with a high degree of central concentration. The core region exhibits a bright, yellowish hue, indicative of an older stellar population. Proceeding outwards from the center, the luminosity gradually decreases, fading into a less defined halo. The overall shape appears mostly rounded, with a slight elongation along one axis suggesting a mild ellipticity. There is no discernible evidence of spiral arms or significant dust lanes. The general morphology indicates a quiescent system, possibly in a later stage of its evolution. There appears to be no interaction with other galaxies or indications of any major merging events disturbing its overall structure. Faint hints of bluer light are seen in the outskirts of the galaxy. 
