The galaxy presents a generally smooth, elliptical morphology, exhibiting high central concentration. The light distribution appears relatively uniform, transitioning smoothly from a bright core outwards. There is a noticeable color gradient, with the central region appearing more yellow-white, suggesting a higher concentration of older stars. Moving outwards, the galaxy becomes slightly redder in hue. There is little evidence of spiral arm structures or dust lanes. The galaxy's shape is nearly circular, though slight deviations from perfect circularity may be present. No obvious signs of recent major merger events are visible, although the possibility of minor tidal disturbances cannot be completely ruled out given the image resolution. The stellar mass appears to be on the higher end, inferred from the luminosity and size of the galaxy. Star formation activity appears to be low, consistent with the older stellar population suggested by the color.
