The galaxy exhibits a roughly elliptical morphology. It has a bright, concentrated central bulge or core region that appears relatively smooth and lacks distinct features. The galaxy's color profile suggests varying stellar populations. The core region presents a bluer hue, potentially indicating the presence of younger, hotter stars, while outer regions exhibit a shift towards redder tones, possibly suggesting older, cooler stars or dust obscuration. There may be some minor disturbances present in the outer disk that could imply a recent gravitational interaction or merging event. It does not appear as if there is a major ongoing merger or collision, but there are some hints of tidal features in the galaxy's outer regions. There may be some star formation regions located away from the core of the galaxy. 
