The galaxy presents a generally smooth morphology, though subtle features hint at underlying structure. The central region exhibits a higher concentration of luminosity, appearing relatively round. There is a slight color gradient, with a bluer hue concentrated towards the central region, and a gradual shift towards redder tones in the outer regions. Faint extensions of light are present, suggesting possible tidal features or minor disturbances. Overall, the galaxy does not exhibit a highly disturbed or actively merging morphology but may have experienced a minor interaction in the past or be currently interacting with a small companion.
