The galaxy presents as a single, concentrated object with a smooth, elliptical morphology. The core exhibits a strong, yellowish-orange color, suggesting a population of older stars. This color is consistent with a galaxy that has undergone significant aging of its stellar population. The lack of discernable spiral arms or a distinct disk structure further supports its classification as an elliptical galaxy. There are no apparent signs of recent or ongoing major mergers, tidal tails, or significant dust lanes. The overall light distribution appears centrally concentrated, gradually fading into the surrounding background, indicating the stellar density decreases from the core outwards. The morphology appears undisturbed, showing no strong indications of current interactions. The galaxy has a red shift of roughly 0.2, indicating it is relatively far from us.
