The galaxy presents a largely smooth morphology, suggesting an elliptical type. It appears quite rounded in shape. There is no strong evidence of spiral arms or a prominent disk structure. The galaxy exhibits a centrally concentrated light profile, with the core appearing significantly brighter than the outer regions. The color is relatively uniform across the galaxy, indicating an older stellar population. No obvious tidal tails, strong dust lanes, or signs of major mergers are visible, however, there may be minor disturbances.
