The galaxy presents a predominantly smooth morphology, appearing largely featureless. Its overall shape is elliptical, exhibiting high degree of roundness. The galaxy displays a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile suggests a population of older stars, potentially with ongoing but moderate star formation. There is no evidence of significant tidal disturbances or ongoing merger activity. Overall, this galaxy appears to be a relatively isolated elliptical galaxy.
