The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The color gradient suggests an aging stellar population dominating the light emission, with a yellow/red hue characteristic of older stars. The galaxy is elongated, exhibiting a cigar-like shape. There is no strong evidence of active star formation regions or spiral arm structures discernible in this image, further suggesting a more passive, evolved system. The overall structure appears undisturbed, lacking any obvious signs of major merging events or tidal distortions. Some minor irregularities are visible, potentially indicative of subtle gravitational interactions or internal dynamical processes.
