The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated light distribution with minimal discernible substructure. The core exhibits a bright, yellowish-orange hue, which gradually fades into the surrounding, less luminous halo. There is no evidence of spiral arms, dust lanes, or significant tidal features, suggesting it is likely a relatively evolved system. The galaxy appears to be roughly circular in projection, deviating only slightly from perfect roundness. There is no clear indication of an ongoing major merger event, although some subtle asymmetries in the outer isophotes cannot be entirely ruled out as minor disturbances. The overall color profile indicates an older stellar population, consistent with a low star formation rate.
