The galaxy presents as a singular, largely featureless object with a smooth morphology. It exhibits a near-spherical shape, deviating minimally from circularity. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. A prominent bulge-like structure is suspected, potentially indicating an elliptical classification. The overall color appears to be dominated by redder wavelengths, suggesting a population of older stars and diminished star formation activity. Any fine details like spiral arms or dust lanes are absent within the limitations of this image's resolution. No signs of major mergers or interactions are visually discernible; there may be slight disturbances. Overall the galaxy is smooth.
