The galaxy presents with a generally smooth, elliptical morphology, though some finer structures are discernable. The core region exhibits high luminosity, appearing almost uniformly bright with a cyan color. Moving outwards from the core, the galaxy displays an extended halo characterized by decreasing surface brightness. There appears to be a slight asymmetrical disturbance to the halo and its surrounding region. There may be some minor merger activity occurring around the galaxy in the surrounding field. Colors transition towards red in the fainter outer regions, indicative of either an older stellar population or increased dust extinction. There also appears to be a relatively undisturbed dust lane or ring around the core of the galaxy. Further spectroscopic analysis is required to resolve stellar populations and chemical composition.
