The observed galaxy presents a predominantly smooth morphology, suggesting an elliptical classification. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. Its shape is moderately elliptical.

There is some evidence of a faint disk-like structure embedded within the larger smooth component, though features are not sharply defined, which is to be expected given the galaxy’s substantial distance. No signs of major mergers or significant tidal disturbances are apparent in this image, although there are subtle hints of minor disturbances. 

The color index suggests the stellar population is relatively old, with a larger population of cooler, redder stars compared to younger, hotter, bluer stars.
