The galaxy presents a predominantly smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity moving outward. The overall shape is approximately round, deviating only slightly from perfect circularity. There are no apparent spiral arm structures or significant dust lanes visible in this image. There is no strong evidence of any major ongoing merger activity or significant tidal disturbances affecting the system. The galaxy exhibits colors that are more red than blue, suggesting a stellar population that is dominated by older stars and a relatively low rate of current star formation. Overall, the galaxy seems to be an elliptical or lenticular type.
