The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The light profile suggests a concentration of older stellar populations. There is no obvious dust lane or spiral arm structure visible in the image. The galaxy displays two distinct regions of light concentration. It is possible this is a merging system, as the overall structure indicates the likelihood of an ongoing or recent gravitational interaction. The colors are consistent with an evolved stellar population, however the slight variation between the two bright regions suggests some minor differences in stellar age or metallicity. There is no evidence of significant ongoing star formation activity. 
