The galaxy presents as an elliptical or lenticular morphology, exhibiting a generally smooth light distribution. It is somewhat elongated in shape, though not highly so. The central region is significantly brighter than the outer edges, which gradually fade into the background. There are no prominent spiral arms or distinct features indicative of active star formation readily apparent. It shows signs of a low to moderate rate of star formation and has an estimated stellar mass in the range of 10^10 to 10^11 solar masses. There appears to be no evidence of a major merger or significant tidal disruption. Minor disturbances cannot be completely ruled out, but are not overtly visible. Overall, the galaxy appears to be a relatively quiescent, evolved system.
