The galaxy presents as a relatively smooth, elongated structure with a subtle bulge. The color profile suggests an evolved stellar population with a concentration in the redder wavelengths, indicative of older stars. One portion has a feature that is more blue, perhaps showing star formation activity. The galaxy appears to be relatively isolated, showing no obvious signs of major tidal interactions or mergers, although there may be some minor disturbance occurring in the bluer region. The overall morphology suggests a system transitioning towards a more quiescent state.
