The galaxy presents as a largely featureless, smooth object. Its morphology appears close to elliptical, exhibiting a high degree of circularity. The color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue, typical for such systems. There is no visible dust lane or spiral arm structure. The apparent absence of significant star formation activity supports the classification as an early-type galaxy. Possible minor disturbances are not readily apparent from the image alone. The galaxy does not visually appear to be undergoing a major merger or significant tidal interaction with another galaxy.
