The galaxy presents an elliptical morphology with a smooth, centralized light distribution, exhibiting a predominantly spheroid structure. There is limited evidence of spiral arms or significant disk features. The galaxy core appears densely packed and intensely bright, with the brightness tapering off smoothly from the center. There is a slight deviation from a perfect sphere, with its light being slightly elongated. There appears to be some minor disturbance or distortion of shape, perhaps caused by a small merger with a dwarf galaxy or gravitational forces from nearby galaxies. The color profile indicates an older stellar population, with redder hues dominating its emission. Overall, the galaxy is a classic example of a mature elliptical galaxy, with its light profile and morphology suggesting an evolved system with limited current star formation.
