The galaxy appears to be a relatively smooth, elliptical system. Its light profile indicates a high degree of central concentration. The color gradient suggests a population of older stars dominating the central bulge, exhibiting a yellowish hue. The galaxy's outer regions appear less concentrated with hints of bluer tones, potentially indicating younger stellar populations. No clear spiral arm structures or dust lanes are discernible. The overall morphology is highly consistent with an elliptical galaxy, possibly with ongoing low-level star formation at the outer edges. There are no obvious signs of a major merger event, though a minor disturbance cannot be completely ruled out at this resolution.
