The galaxy presents as a relatively smooth, centrally concentrated object. Its apparent shape is elliptical, exhibiting a moderate degree of roundness, with the majority of observers agreeing it falls somewhere in between completely round and elongated.  The light distribution appears fairly uniform across the galaxy, with a subtle color gradient, shifting from a bluer hue at its core to redder tones in the outer regions. There is no strong evidence of spiral arms, a prominent bulge, or any significant disk features. The galaxy appears largely undisturbed, showing no clear signs of major mergers or tidal disruptions, with the vast majority of classifications suggesting no ongoing merging activity, though some do indicate a possibility of minor disturbances.  This galaxy is estimated to be a moderate mass object with a low rate of star formation.
