This galaxy exhibits an elliptical morphology with a smooth, concentrated central bulge. The light distribution appears relatively uniform, suggesting an older stellar population. There's a subtle color gradient, with the core appearing more yellow, possibly indicating a higher concentration of older, redder stars, with less of the blue spectrum. The isophotes are generally round with a lack of discernible spiral arm structure or prominent dust lanes. There is a lack of morphological distortion or obvious signs of major merger activity. Overall, this appears to be a quiescent elliptical galaxy.
