The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge with a gradual falloff in luminosity toward the edges. The galaxy appears nearly circular in projection, displaying minimal evidence of strong spiral arm structures or significant tidal disturbances. The color is predominantly yellowish-white, suggesting an older stellar population and relatively low ongoing star formation. There is faint evidence of minor disturbances or asymmetries, but not strong enough to identify the galaxy as undergoing a major merger event.
