The galaxy presents a largely smooth and rounded morphology, exhibiting characteristics consistent with an elliptical or lenticular galaxy type. There is a slight, but visible, disk-like feature. The galaxy is dominated by a bright central bulge, with a gradual decrease in luminosity towards its outer edges. Color gradients are subtle, showing a bluer tint towards the central region, suggesting the presence of younger stellar populations or ongoing star formation activity within that area. There is little evidence of strong spiral arms or significant dust lanes. The overall structure appears relatively undisturbed, with minimal signs of major mergers or tidal interactions. There is an absence of a strong, actively galactic nucleus. Based on the observed features, this galaxy likely has a stellar mass slightly above 10^9 solar masses. The galaxy shows weak star formation activity.
