The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a lack of prominent spiral arms or distinct disk structures. A diffuse halo extends outwards from the bright central region, gradually fading into the background. There are no indications of significant tidal disturbances or ongoing major mergers, although subtle asymmetries could potentially indicate minor gravitational interactions. Color gradients suggest a slightly redder core compared to the outer regions.