The galaxy presents as a largely smooth, elliptical structure. Its core exhibits a concentrated, luminous orange hue, suggesting an older stellar population dominating the central region. The luminosity decreases radially outwards, transitioning into a diffuse, yellowish halo. There is little evidence of distinct spiral arms or significant dust lanes. The overall shape appears close to round with a slight elongation, though not significantly cigar-shaped. No obvious signs of major mergers are apparent in the image, although a minor disturbance cannot be ruled out.
