The galaxy presents as a relatively smooth, elliptical-shaped object. Its core appears quite bright and concentrated, emitting a yellowish-orange hue that suggests an older stellar population. A broader, less intense halo surrounds the core with a faint greenish tint, possibly indicative of some ongoing, low-level star formation. There is no obvious presence of a prominent disk structure or spiral arms. Faint disturbances may be present on the edges. The galaxy's shape is more in between elliptical and round, rather than highly elongated or perfectly spherical. There is no strong visual evidence of major mergers or significant tidal disturbances affecting its overall morphology.
