The galaxy presents as an elliptical or lenticular morphology, appearing mostly smooth with a slight elongation. There is a lack of distinct spiral arm structure or prominent dust lanes. The color gradient indicates a central region that is more yellow/gold in hue, suggesting an older stellar population. The outer regions of the galaxy appear slightly bluer. The galaxy appears undisturbed with no clear evidence of major tidal interactions or ongoing mergers. It is relatively compact, with a moderately high mass. The star formation rate is quite low. 
