The galaxy appears to be a disk galaxy, viewed at a high inclination. The central bulge is prominent and shows a bright, nearly unresolved core, which may suggest the presence of an active galactic nucleus. There's a clear color gradient visible, transitioning from bluer hues in what appears to be the outer disk to redder tones closer to the bulge. The disk shows some subtle features, possibly faint spiral arm structures, but its smoothness predominates, with the majority of its light emitted at the bluer end of the spectrum. The galaxy's overall morphology indicates it is not currently undergoing a major merger or significant tidal interaction, though minor distortions or asymmetries cannot be ruled out. Its elliptical shape suggests a spheroidal component with a moderate amount of flattening.
