This galaxy presents a predominantly smooth and rounded morphology. There appears to be a central bright region, potentially indicating a dense concentration of stars or an active galactic nucleus. The light distribution suggests a spheroidal shape, with a gradual decrease in intensity moving outwards from the core. There is a slight extension of blueish light surrounding the central region, suggestive of ongoing or recent star formation. No distinct spiral arms or bar structures are discernible within the resolution of the image. Overall, the galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions with neighboring galaxies. The galaxy's color profile leans towards the redder end of the spectrum in the inner regions and bluer in the outer regions.