The galaxy presents an elliptical morphology. It appears largely smooth with a concentrated central bulge, showing a transition in color from a redder core to a bluer halo. The galaxy's elongated shape suggests it is more cigar-shaped than round. There is no evidence of strong tidal features or major disturbances from interactions, though minor irregularities may be present. The galaxy's redder core indicates an older stellar population, with the bluer halo suggesting more recent, ongoing, or recent star formation. The galaxy exhibits a color profile consistent with a system that is undergoing some level of star formation despite its overall smooth and relatively undisturbed appearance.
