The object in question appears to be an elliptical galaxy, exhibiting a largely featureless and smooth morphology. It possesses a high degree of central concentration, with a luminosity profile that gradually fades outwards from the core. The galaxy's overall shape is consistent with a spheroidal structure, showing a high degree of circularity, though the possibility of a slight elongation cannot be entirely ruled out. Its color indices suggest an older stellar population, indicative of a low ongoing star formation rate. There is no visible evidence of spiral arms, dust lanes, or any signs of recent or ongoing mergers or tidal disturbances. The galaxy's apparent size is small, suggesting it is at a considerable distance.
