The galaxy exhibits a generally smooth morphology, appearing as a diffuse, spheroidal structure. The light is concentrated towards the center, indicating a prominent nucleus or bulge. The galaxy displays a yellowish hue in its central region, potentially indicative of an older stellar population. There is no evidence of spiral arms or a prominent disk. Subtle color variations are observable, but overall, the light distribution is smooth and continuous, with a gradual decrease in intensity from the core outwards. There is no observed disturbance indicating a merger. The overall shape is round.
