The galaxy appears as a centrally concentrated, smooth elliptical with a rounded morphology. The color profile is generally yellowish, suggestive of an older stellar population. There is a slight elongation, but overall the galaxy is largely spheroidal. No distinct spiral arms or bar structure are discernible. The image does not indicate any significant tidal disturbances or obvious signs of an ongoing merger event, though minor disturbances cannot be ruled out given the image resolution. The light is concentrated towards the center and smoothly diffuses outward, suggesting a lack of significant dust lanes or active star formation regions.
