The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round and featureless at this resolution. There are no apparent spiral arms or a distinct disk structure evident. The light distribution appears to decrease steadily from the core outwards. The core region is brightest and takes on a yellow-white color, indicative of older stellar populations. A slightly bluer halo surrounds the brighter core, suggesting the presence of some younger stars or perhaps lower levels of ongoing star formation in the galaxy's outer regions, but overall star formation is generally low. There is no evidence of any major merger events or significant tidal disturbances in the vicinity. Some very minor irregularity in shape may be present upon closer inspection, but this would need to be verified with additional data.
