The galaxy presents as a relatively smooth, disk-like structure with an apparent red-shift. The light distribution suggests a concentration of older stellar populations, potentially indicating an elliptical or lenticular morphology, but with subtle features suggesting a disk component. There is little indication of prominent spiral arms or active star-forming regions. The overall color suggests a paucity of young, massive stars. The galaxy exhibits a slight elongation, which may be evidence of a disk viewed at an angle. Overall, it appears to be a galaxy undergoing passive evolution.
