The galaxy appears to be an elliptical type, exhibiting a smooth, elongated profile reminiscent of a cigar shape. There's a concentration of light towards the center, suggesting a prominent galactic bulge. The color gradient transitions from a yellowish core to a bluer periphery, implying differing stellar populations across the galaxy. Given the smooth texture and lack of readily apparent spiral arms or dust lanes, it’s likely that star formation is either low or has largely ceased within this system. No major distortions or tidal features are visible, suggesting it is not undergoing a major merger event. There might be some minor disturbances, but further examination would be required to confirm these features. The light is most concentrated along the central axis.
