The galaxy presents as a relatively smooth, elliptical shape with a noticeable cigar-like elongation. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue. The overall color gradient suggests an older stellar population, with the outer regions showing a slightly redder tint. There's minimal evidence of significant disk structures or spiral arms. Subtle irregularities along the edges may indicate minor disturbances or interactions, but no major merging events are apparent from the image.
