The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution with little discernible spiral structure or distinct features. The overall shape is elongated, but nearly circular. The galaxy is dominated by older stellar populations, with a color profile trending towards redder hues. There is no evidence of significant ongoing star formation in the visible bands, but there may be a small region of blue light on one side of the galaxy, which could indicate a slight disturbance or region of increased star formation in a small area. The galaxy shows no strong signs of a recent major merger or tidal disruption. There appears to be a smooth, even decrease in light as you move from the center of the galaxy to the outer regions.
