The galaxy presents as a relatively smooth, elliptical or lenticular form. It exhibits a concentrated, round morphology with minimal discernible structure in the visible light spectrum. The galaxy appears to be dominated by an older stellar population, indicated by its redder hue, characteristic of evolved stars. There is some evidence of possible minor gravitational disturbance occurring within the galaxy. The smoothness of the light distribution suggests that any major merging events have occurred in the distant past or that the object is still in the process of merging. The galaxy appears to have a low star formation rate. 