The galaxy appears to be relatively compact and luminous. The morphology is dominated by a smooth, spheroidal component. There is a slight elongation but it mostly appears round. Possible tidal features are subtle, but there could be faint disturbances indicative of past or ongoing interactions, particularly in the form of diffuse light around the main body. There may be some evidence of merging galaxies. The color profile suggests a gradient from a more reddish core to slightly bluer outer regions, though the resolution makes this difficult to discern. There are no clear spiral arm structures visible. Overall, the galaxy resembles an elliptical or S0 type galaxy, showing signs of potential past interactions.
