The galaxy appears to be a relatively smooth, centrally concentrated object. The light profile suggests a dominant bulge component, giving it an elliptical or lenticular morphology. There is a possible faint disk surrounding the bulge. The galaxy's color profile indicates a redder central region, which could be attributed to an older stellar population or dust obscuration. The outer regions of the galaxy exhibit a bluer color, hinting at the presence of younger stars or ongoing star formation, though at a low rate. There are no clear signs of major disturbances. The overall appearance suggests a galaxy undergoing a transition from active star formation to a more quiescent state.
