The galaxy presents as a somewhat elongated, elliptical form. The central bulge exhibits a concentrated and relatively bright emission, appearing orange in color. Surrounding the bulge, a broader disk is apparent, characterized by a greenish hue. The shape of the galaxy is clearly elongated, with a major axis significantly longer than its minor axis. There is no strong evidence of spiral arm structures or significant dust lanes within the galaxy's structure. The galaxy appears relatively smooth overall with a slight amount of disturbance to its appearance. The color gradient suggests a concentration of older stellar populations in the central bulge and perhaps more recent star formation in the surrounding disk. There is no strong indication of any major ongoing merger activity or strong tidal features.
