This galaxy presents an ellipsoidal morphology, exhibiting a relatively smooth overall structure. A central bulge region is clearly visible, characterized by a brighter, concentrated light profile. The outer regions of the galaxy display a more diffuse appearance, with hints of a flattened disk-like structure but lacking well-defined spiral arms. The galaxy's color suggests a mix of stellar populations, with a generally bluish hue, although the colors are subdued, possibly indicating a relatively low ongoing star formation rate. There is evidence of some disturbance in the galaxy's morphology, hinting at the possibility of a past interaction or merger event. The galaxy is neither perfectly round nor extremely elongated.
