The observed galaxy presents an intermediate morphology, exhibiting characteristics of both smooth and featured galaxies. The central region is dominated by a smooth, concentrated bulge with a yellowish hue, suggesting an older stellar population. Extending outward from the bulge, there is evidence of a faint, disk-like structure, although its features are not sharply defined. There is also a hint of a spiral arm or tidal tail emanating from one side of the galaxy, indicating possible gravitational interaction or recent merger activity.

The overall color gradient transitions from the yellowish core to bluer outskirts, implying ongoing star formation in the outer regions. Irregularities and a slight asymmetry in the galactic shape are present, pointing towards a potential minor disturbance due to a past interaction. The galaxy does not appear to be undergoing a major merger, but subtle signs indicate that it is not entirely undisturbed.
