The galaxy exhibits a morphology suggestive of a system undergoing or having recently undergone a merger or interaction. The primary component displays a generally smooth light distribution with a concentration towards the center. There is a secondary concentration of light nearby. Overall the system has an irregular shape.
The color of the light emitted from the galaxy indicates a population of older stars. The galaxy displays a yellowish hue, which suggests that the stellar population is not dominated by young, hot, blue stars associated with active star formation. Some evidence of limited on-going star formation may be seen.
Based on the observed characteristics, this galaxy is potentially an elliptical or lenticular galaxy.
