The galaxy presents as a relatively compact object, approximately circular in appearance. Its color profile indicates a concentration of light in the yellow-red wavelengths, suggesting a population of older stars and potentially a relatively low rate of current star formation. The galaxy exhibits a smooth morphology, lacking prominent spiral arms or distinct features, which may indicate a classification towards the elliptical end of the Hubble sequence or a lenticular galaxy. There may be signs of a minor disturbance or a possible interaction or recent merger event, particularly an asymmetrical feature that could be tidal debris. Overall, the appearance implies an evolved system of intermediate mass. 
