The galaxy presents a largely smooth and rounded morphology, with a concentrated central bulge exhibiting a bright, pale yellow color. Diffuse, bluish regions extend outwards from the bulge, suggesting the presence of ongoing star formation activity. The galaxy displays a slight distortion or asymmetry in its overall shape, hinting at potential past interactions or minor disturbances. The structure lacks any obvious spiral arms or a well-defined disk, possibly indicating an elliptical or lenticular classification. The galaxy appears relatively compact, with a moderately high mass and a low specific star formation rate.
