The galaxy appears to be a relatively compact system, exhibiting an elliptical or lenticular morphology. The core is intensely bright and concentrated, displaying a pronounced yellowish-orange hue, suggesting a significant population of older stars. The surrounding halo is less defined and appears smoother, with a faint greenish tint towards the outer edges. There is evidence of possible tidal interaction or a minor merger event visible as a small plume extending from the main galactic body. The color gradient suggests some degree of ongoing or recent star formation, particularly in the regions with a greenish hue, though the overall star formation rate appears to be relatively low. The system is fairly massive, with a smooth light distribution. There also seems to be a minor disturbed fraction on the left side of the galaxy, and possibly undergoing a merging event. 
