The galaxy presents as a single, largely featureless object with a concentrated central region. The light profile appears smooth and spheroidal, with a gradual decrease in intensity from the core outward. Color gradients are subtle, with a tendency towards redder hues concentrated within the central region, suggesting an older stellar population. There is no apparent spiral structure or disk component visible, nor any signs of ongoing major mergers or tidal disturbances. The overall morphology is consistent with an elliptical galaxy, potentially at a significant distance given the object's angular size.
