The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge, a fainter, bluer halo is visible, possibly indicative of ongoing, though subdued, star formation within the outer regions. The overall shape is nearly round, with only a slight deviation from perfect circularity. There is no strong evidence of spiral arms or significant disk structures. The galaxy shows no obvious signs of major mergers or tidal disturbances, although there is a hint of some minor irregularity in the outer halo, possibly due to a past interaction. The galaxy appears relatively compact, with a moderate angular size in the image. Overall, this galaxy appears to be a quiescent, evolved system with limited ongoing star formation.
