The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless in this image. There is a centrally concentrated, bright, and slightly elongated core. The color of the core appears to be skewed towards the redder end of the spectrum. The galaxy's light gradually diminishes from the center outwards, with no apparent spiral arm structures or prominent dust lanes visible. There appears to be only a small amount of blue light surrounding the edges of the core. The overall impression is one of a relatively evolved system, potentially with an older stellar population dominating its light output. Based on the slight elongation, the galaxy does not appear to be perfectly spherical, but rather somewhat ellipsoidal. No obvious signs of recent major merger activity, such as tidal tails or strong distortions in the shape, are readily apparent, however there is a slight irregular shape.
