The galaxy presents a generally smooth, elliptical morphology. It exhibits a central bulge that is bright and concentrated, with a gradual decrease in luminosity towards the outer regions. The color profile appears relatively uniform, with a slight shift towards redder hues in the central region. There is a subtle hint of a disk component, but it is not well-defined. No distinct spiral arms are visible, and the galaxy lacks any significant dust lanes or prominent star-forming regions. Based on its shape, it is likely an elliptical galaxy with ongoing star formation. The overall structure suggests a relatively relaxed system, potentially in a later stage of its evolution. There is some indication of minor disturbances in the galaxy's morphology.
