The galaxy presents a generally smooth morphology with little apparent substructure. Its shape is elongated, appearing somewhere between round and cigar-shaped, but closer to being in between. The galaxy exhibits a color gradient, with a slightly bluer hue toward the central region and a gradual shift towards redder colors in the outer regions. This color variation could indicate differences in stellar populations or dust content across the galaxy. There is no obvious evidence of ongoing major mergers or strong tidal disturbances, suggesting a relatively undisturbed evolutionary history. Possible presence of minor disturbances that needs further investigation.
