The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The core region displays a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the light gradually fades into a reddish halo. While the overall shape seems roughly circular, there is a slight elongation, indicating a possible deviation from a perfect sphere. No distinct spiral arms or dust lanes are readily apparent. There are subtle indications of minor disturbances, but no major merger events seem to be impacting the morphology. Overall, the galaxy's structure is dominated by a smooth, evolved stellar population.
