This galaxy exhibits a relatively smooth morphology, appearing as a spheroid with a high degree of roundness. There is little evidence of prominent spiral arms or a well-defined disk structure. The galaxy displays a primarily red-shifted color, possibly indicating an older stellar population and lower current star formation rate. There are suggestions of a very minor disturbance, perhaps a faint tidal tail or asymmetry in the outer halo. Any merger history would be in the very distant past. Overall, the galaxy appears to be a fairly quiescent system, likely an elliptical galaxy that is not actively undergoing significant star formation.
