The galaxy appears as a relatively compact and luminous object. The light distribution is largely smooth and centrally concentrated, with a round shape. There is little to no visible disk structure or spiral arm features. A slight color gradient is observable, with the central regions exhibiting a yellowish hue, suggesting a population of older stars. The outer regions appear slightly bluer, though still relatively quiescent. Signs of major mergers or significant tidal disturbances are absent. Faint extensions or very minor irregularities might be present upon closer inspection but could be noise. Overall, the galaxy presents as a well-evolved system with low recent star formation activity.
