The galaxy presents a predominantly smooth, elliptical morphology. It appears nearly round in shape, with a slight deviation towards a less circular form. There is a central concentration of light, suggestive of a galactic nucleus, though distinct features such as spiral arms or a prominent disk are not readily discernible. The color gradient exhibits a general trend towards bluer hues at the periphery, potentially indicating younger stellar populations in the outer regions, with a shift towards redder colors in the core, possibly due to older stars and dust. No significant signs of ongoing or recent major mergers are evident, although subtle irregularities might suggest minor interactions or disturbances.
