The galaxy presents a generally smooth, elliptical morphology. The core appears bright and concentrated, exhibiting a yellowish-orange hue. This suggests an older stellar population within the central bulge. There is a subtle color gradient, with the outer regions showing a slight shift toward redder tones. The isophotes are generally regular and concentric, indicating a relaxed and well-mixed system. No distinct spiral arms or prominent dust lanes are visible. Overall the image appears to depict a single isolated galaxy. There is no visible evidence of significant ongoing star formation.
