The galaxy presents as a moderately bright, elliptical-shaped object, displaying a relatively smooth and symmetrical morphology. A dominant central bulge exhibits a higher surface brightness concentration, gradually decreasing towards the outer regions of the galaxy. The color appears predominantly bluish, suggesting the presence of a younger stellar population and ongoing star formation, albeit at a moderate rate. There is a slight indication of a flattened disk component, though it is not distinctly defined. There are no prominent spiral arms or obvious signs of recent major merger events. Small disturbances or minor irregularities are not entirely absent, implying potentially subtle interactions or past minor mergers. The overall appearance suggests an intermediate-mass galaxy that is likely undergoing a period of relatively quiescent evolution, transitioning towards a more spheroidal configuration.
