The galaxy appears as a flattened, elliptical structure. Its morphology indicates a smooth, cigar-like shape with a high degree of symmetry. There is a bright central bulge that fades outward into a less defined disk. The overall color is yellowish-white, suggesting an older stellar population with relatively little active star formation, though subtle blue-ish tinges on the edges of the galaxy suggest possible regions of on-going or recent star formation. No distinct spiral arms or bars are visible in the image. There is no major distortion, and no indication of ongoing merger activity. A minor disturbance might be occurring at one end of the galaxy. Overall, the galaxy seems to be a relatively isolated system that appears to be in a relatively late stage of evolution.