The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color profile suggests a mixture of stellar populations, with some regions exhibiting bluer hues indicative of younger, hotter stars, and other areas appearing redder, likely composed of older, cooler stars. There is a slight elongation to the morphology, not quite spherical but also not a highly flattened disk. Faint features, perhaps indicative of spiral arms or tidal disturbances, are subtly present, although not sharply defined. The general appearance points towards an intermediate stage between a pure elliptical and a well-defined spiral galaxy. No particularly dominant or active galactic nucleus is apparent from the image. There may be some ongoing, low-level star formation activity.
