The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a predominantly elliptical morphology, exhibiting a high degree of radial symmetry. A bright central bulge is clearly visible, surrounded by a more diffuse halo of light. There is a subtle color gradient, with the core appearing slightly bluer than the outer regions. No distinct spiral arms or significant dust lanes are apparent, supporting the classification as an elliptical galaxy. Minor asymmetric features suggest a past, or potentially ongoing, minor interaction or disturbance. The overall structure indicates a gravitationally relaxed system, consistent with an older stellar population and a low star formation rate.
