This galaxy presents as an elliptical morphology, appearing mostly smooth and rounded in shape. The light distribution suggests a concentration of older stellar populations towards the core, indicated by the yellow-orange hue, with potentially ongoing, though relatively subdued, star formation activity. The slight hints of bluer colors at the periphery may indicate the presence of younger, hotter stars within the extended galactic halo. There's a suggestion of minor disturbances in the galaxy's form, but it appears to be largely isolated with no obvious signs of major interactions or mergers occurring. Overall, this galaxy presents as a fairly massive, evolved system undergoing a relatively quiescent phase.
