The galaxy presents as a somewhat irregular, though generally smooth, structure. There is a dominant central bulge. The overall shape is neither perfectly elliptical nor spiral, with a hint of disturbed morphology, possibly indicating an ongoing or past interaction with another galaxy. Color gradients suggest a relatively old stellar population, particularly concentrated in the central region which appears more yellow. The outer regions exhibit a bluer hue suggesting the presence of younger, hotter stars, but with a low rate of overall star formation. The galaxy displays a moderate degree of spatial extent with a measured effective radius of approximately 3.8 kpc. There are areas of lower surface brightness surrounding the central core, indicating a more diffuse halo.
