This galaxy presents a generally smooth, elliptical morphology. Its light distribution appears concentrated towards the center, with a gradual decrease in intensity outwards. There is a lack of apparent spiral arms or a prominent disk structure. The galaxy exhibits a mostly round shape, with slight deviations towards a more intermediate form. There is no evidence of significant ongoing merging activity or major tidal disturbances. The color index suggests a population of relatively older stars with limited current star formation. The overall appearance is consistent with an early-type galaxy at a considerable distance.
