The galaxy presents a generally smooth morphology, with a centrally concentrated brightness profile, but is visibly disturbed. There appears to be evidence of possible tidal features or distortions extending from the main galactic body, though the detail is quite limited. The galaxy exhibits a bluer central region, likely indicating a higher concentration of younger, hotter stars or recent star formation in the nuclear region. The outer regions appear redder, suggesting an older stellar population. There is a slight elongation in the galaxy's shape. Overall, the galaxy exhibits a mix of smooth and irregular features, with an apparent disturbance.
