The galaxy presents as a moderately compact object with a somewhat smooth overall morphology. There is a slight suggestion of a central concentration, however, distinct features such as spiral arms or a prominent bar structure are not readily apparent. The galaxy displays a subtle blue hue, potentially indicative of ongoing or recent star formation activity, although the rate appears to be relatively low. The galaxy's shape is somewhere between round and elliptical. There is some evidence of minor disturbances, however the overall shape is not significantly disrupted suggesting a relatively stable system. There is no clear indication of a major merger event in its recent history.
