The galaxy presents a generally smooth morphology with subtle features. It appears largely rounded in shape, with a hint of elongation suggesting it is not perfectly spherical. There is evidence of internal structure within the galaxy, potentially a very diffuse and faint disk-like feature, although the smoothness dominates. The galaxy exhibits a redder hue than the other objects within the frame, potentially indicating an older stellar population, as the star formation rate appears low. The tidal interaction and merger is evident as an overall disturbed morphology and slight asymmetries in the light distribution, although not highly prominent. There may be some faint wisps or extensions indicative of past merger activity, but these are very subtle and could also be artifacts of imaging. 
