The galaxy presents a generally smooth and rounded morphology, with a concentrated central region.  There is some indication of a slight elongation, although the overall shape remains largely circular. The galaxy exhibits a color gradient, appearing bluer towards the center and becoming redder in the outer regions. There are no discernible spiral arms or prominent dust lanes. There is a slight asymmetry, and it is possible that the system has experienced some tidal disturbances. The overall light distribution suggests a relatively evolved stellar population.
