The galaxy appears to be elliptical in shape, presenting a largely smooth morphology with a slight elongation. A concentrated central bulge exhibits a bright, almost uniformly white appearance, suggesting a high density of older stellar populations. The galaxy's light profile fades gradually outwards from the core. There is a hint of a faint blue-ish feature on one side, perhaps indicating a small region of younger stars or an area of ongoing star formation. Overall, the galaxy lacks prominent spiral arms or strong dust lanes, further supporting its classification as an elliptical galaxy. It does not appear to show any strong signs of interaction or merging with another galaxy, with no significant tidal tails or distortions observed. 
