The galaxy presents as a centrally concentrated, relatively smooth object with a noticeable spheroidal morphology. The core exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, the galaxy displays a gradual decrease in surface brightness. The overall color gradient indicates a shift towards bluer hues in the outer regions, possibly due to the presence of younger, hotter stars. No distinct spiral arms or bar structures are discernible; instead, the light distribution appears relatively uniform and unstructured. The galaxy exhibits an approximately elliptical shape, with a slight deviation from perfect circularity. There are no readily apparent signs of major mergers or significant tidal disturbances, although subtle irregularities in the outer regions cannot be entirely ruled out at this resolution.
