The galaxy appears to be an elliptical galaxy, displaying a smooth, featureless morphology. It has a cigar-shaped profile, elongated along a major axis. A bright central bulge is visible, with the luminosity gradually decreasing towards the outer edges. Color gradients suggest that the bulge may contain older stellar populations, while the outer regions exhibit a bluer hue. No spiral arms or dust lanes are apparent. The overall structure implies that any recent merger events were likely minor disturbances in the galaxy's history.
