The galaxy presents a generally smooth morphology, with a slightly elongated or elliptical shape. There may be some minor disturbances in the structure, but the overall appearance is not strongly disrupted. The galaxy exhibits a color gradient, with the central region appearing more yellow/orange, possibly indicating an older stellar population or significant dust obscuration. The outer regions show a hint of bluer colors, suggesting the presence of some younger, hotter stars. There may be evidence of some recent star formation, although it appears to be relatively quiescent at the current epoch. The galaxy is relatively massive, indicating a substantial stellar content. The morphological classification suggests a transition between a smooth elliptical galaxy and a galaxy with some disk-like features or disturbances.
