The galaxy appears as a single, relatively smooth object with a high degree of circular symmetry. The light distribution is centrally concentrated, with a gradual decrease in intensity outwards. The galaxy exhibits a color gradient, transitioning from a slightly bluer core region to redder outer regions. There is no evidence of spiral arms or a distinct disk component, which suggests that it is likely an elliptical galaxy. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although the low image resolution prevents identification of subtle irregularities. Based on the observed color and morphology, the stellar population appears to be primarily composed of older stars, which is consistent with a low rate of recent star formation. 
