The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. Its core region presents a strong, yellowish luminosity, possibly indicating an older stellar population. Moving outward from the core, the light diffuses into a broader, less intense halo. The galaxy's color gradient suggests a transition from older stars in the center to a mix of stellar ages in the outer regions. There is a slight asymmetry in the outer light distribution, which could indicate a past minor interaction or a faint disk component viewed at an angle. Overall, the galaxy presents as a well-defined, relatively undisturbed system.
