The galaxy presents an elliptical morphology, appearing as a flattened spheroid. Its central region exhibits a concentrated, bright yellowish-white luminosity, suggestive of an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in brightness. Subtle color variations are present, with hints of blue-green in the outer regions, potentially indicating pockets of younger, hotter stars or ongoing star formation. A slight distortion in its otherwise smooth structure may be indicative of minor gravitational interactions or recent accretion events. Overall, the galaxy appears as a relatively evolved system with subdued star formation activity.
