The galaxy presents an elliptical morphology, though some distortions are present. Its core exhibits a bright, concentrated luminosity, which suggests a high stellar density and possibly an active galactic nucleus. The overall color is yellowish-white, indicative of an older stellar population, although some bluer regions are present. The shape appears to be approaching a round structure, however, it appears slightly elongated. There is potential evidence of tidal disturbances or interactions, indicated by faint streams or diffuse structures extending from the primary galactic body. These features hint at past or ongoing merger activity.
