The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated luminosity, gradually fading into the outer regions. The object appears elongated, but significantly deviates from a cigar shape. There is a slight color gradient within the galaxy, exhibiting a slightly redder hue at its core, slowly transitioning into a bluer color in its faint outskirts. Evident signs of a major disturbance, such as tidal tails or prominent asymmetries, are absent from the galaxy's structure. Close inspection reveals the possibility of minor disturbances, but nothing obviously suggesting an ongoing merger. This galaxy appears to be a fairly typical example of an elliptical galaxy observed at a cosmological distance.
