The galaxy presents a predominantly smooth morphology, with an apparent lack of defined spiral arms or a prominent central bar. The light distribution suggests an elliptical or lenticular classification. There is a notable concentration of light towards the center, indicating a bulge component. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly circular. Faint, diffuse features are present in the outer regions, hinting at potential tidal interactions or past merger events. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the yellower core. Based on these observations, the galaxy is likely a relatively massive system, possibly undergoing or having undergone significant star formation activity.
