The galaxy appears to be a relatively compact and luminous system, with an estimated effective radius on the order of 4 kiloparsecs. Its overall morphology is predominantly smooth, with a subtle hint of distortion. The light profile indicates a generally well-mixed stellar population.

The galaxy exhibits a color gradient, with a slightly bluer color in the outer regions transitioning to a redder core. This could imply ongoing or recent star formation in the outskirts, or varying metallicities within the galaxy. There appears to be a possible tidal feature, which is indicative of recent or ongoing interactions with another galaxy. This feature may be related to some observed disturbance, or a potential merger event.