The galaxy presents a generally smooth and rounded morphology. The light distribution appears centrally concentrated, exhibiting a gradual decrease in intensity from the core towards the outer regions. There is very little to no evidence of spiral arms or a disk structure in the galaxy. The overall color appears to be redder, which may indicate a population of older stars. No signs of tidal disturbances, major mergers, or interactions with other galaxies are readily apparent. The light appears mostly smooth and featureless.
