The galaxy appears to be a relatively smooth, elliptical galaxy. It is centrally concentrated with a bright, yellowish core, which likely indicates an older stellar population dominating the central region. The galaxy fades gradually outwards, with the outer regions appearing bluer in color, suggesting the presence of some younger, bluer stars. It is elongated in shape, appearing more 'in between' in terms of roundness, with little to no signs of spiral arms or a distinct disk structure. There is no obvious evidence of recent major mergers or significant disturbances in the galaxy's structure, although there may be a slight asymmetry in the outer regions. Overall, the galaxy seems relatively undisturbed and exhibits a relatively normal elliptical morphology.
