The galaxy presents a relatively smooth morphology, exhibiting a predominantly elliptical shape. There is a slight elongation. The galaxy's color profile suggests a population of older stars, with a redder hue dominating the overall light emission. There is a lack of distinct spiral arm structures or prominent dust lanes, reinforcing the classification as an elliptical galaxy. There is no evidence of active galactic nuclei or intense star formation regions, implying a quiescent or passively evolving state. No merging or tidal disturbances are visible in this image. The galaxy's structure is fairly uniform in luminosity with a slightly brighter center, though no evidence of any bar structure is apparent.
