The galaxy exhibits a mostly smooth morphology, suggesting an elliptical or lenticular classification. Its shape appears somewhat elongated, but not highly so. There is a prominent central bulge exhibiting a yellowish-white hue. The outer regions of the galaxy show a subtle disk-like structure and a faint greenish-blue tint, potentially indicative of some ongoing, albeit low-level, star formation. There is also a small amount of red present, possibly indicating older stars or dust. There is no obvious evidence of major mergers or tidal disturbances.
