The galaxy presents a predominantly smooth morphology. It appears nearly circular in shape, with a slight deviation towards an intermediate elliptical form. There is no discernible spiral structure or bar. The galaxy exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards its outer regions. A subtle color gradient is observed, transitioning from a brighter, slightly bluer core to a more subdued, redder halo. There is no clear evidence of significant tidal disturbances or ongoing major mergers, though subtle asymmetries might suggest minor interactions.
