The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. Its overall shape is somewhat elongated, leaning towards a cigar-like form. The light distribution appears concentrated towards the center, indicating a dense galactic nucleus. The color gradient suggests a population of older stars, with a reddish-yellow hue dominating the core region, fading to a bluer color further from the center. There is no visual evidence of spiral arms or dust lanes, suggesting a relatively quiescent state with a low star formation rate. There is no major disruption in its structure, suggesting there is no major merger occurring, but a small minor disturbance cannot be ruled out.
