The galaxy appears to be a relatively smooth, elliptical-like structure. Its shape is elongated, showing a moderate cigar shape. There is a slight disturbance in its morphology, potentially indicating a minor interaction or internal activity. The galaxy has a distinct central core that shows a gradual decrease in luminosity towards the edges, suggesting an even distribution of light across the galaxy. It appears to be a non-merging system, and there is little evidence of strong recent star formation.
