The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light profile. There is a bright, yellowish core, indicative of an older stellar population. A faint blueish disk can be observed, revealing that this is likely a lenticular or spiral galaxy. The overall color gradient suggests a transition in stellar populations, with older stars concentrated in the core and a disk of younger stars in the spiral arms. It does not appear to be undergoing any major merging events, but there are some disturbances in the light distribution that could be the results of a minor merger. 
