The galaxy presents a relatively smooth, elliptical morphology. It is elongated in shape, appearing cigar-shaped, with a diffuse, extended halo. The central bulge is prominent, displaying a concentrated luminosity. No distinct spiral arms or features are discernible. There is a noticeable color gradient, trending from a slightly bluer periphery to a redder, more concentrated core. The overall structure suggests a lack of significant ongoing star formation. There is no evidence of active galactic nuclei or dust lanes. Any tidal disturbances or indications of recent mergers are minimal. The galaxy is primarily classified as a smooth galaxy.
