The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, indicative of a substantial stellar population and/or active galactic nucleus. The galaxy's color is predominantly yellowish-orange, suggesting an older stellar population and a relative lack of ongoing star formation. There are no apparent spiral arms or significant dust lanes visible. The galaxy is generally round in appearance, showing no significant elongation or tidal distortions that would suggest recent merger activity or significant external gravitational influence. Faint, diffuse light extends outwards from the central region, but the overall structure lacks defined features.
