The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-white, suggesting an older stellar population in the core. The galaxy displays a gradual decrease in luminosity moving outwards from the center. There's a subtle color gradient, with the outer regions appearing slightly bluer, hinting at the presence of younger stars or ongoing star formation, although this is not very pronounced. No distinct spiral arms or bar structures are discernible in the image. The overall structure appears undisturbed, showing no signs of major mergers or tidal disruptions. The galaxy seems to be relatively isolated, with no immediately apparent companion galaxies.
