The galaxy presents a generally smooth morphology. It appears moderately elliptical, neither perfectly round nor highly elongated. There may be a slight disk like feature, but not very prominant. The central bulge is subtly brighter and more concentrated than the outer regions. There is potentially some slight disturbance or merging activity occurring, although definitive tidal tails or strong distortions are not apparent. The galaxy appears somewhat massive, with a substantial stellar population. The colors suggest a population with a wide range of stellar ages, but it is more heavily weighted towards redder colors suggesting that it could be old. There might be a small ammount of active star formation occurring.
