The galaxy presents an elongated, somewhat disturbed morphology. There is an area of more concentrated light near the center of the galaxy, exhibiting a diffuse yellowish hue, indicating the presence of older stellar populations. Extending downwards from the center is a fainter, elongated arm or tail showing hints of blueish light. This suggests the presence of younger, hotter stars, potentially indicative of ongoing or recent star formation within this region. The galaxy does not appear to exhibit a well-defined spiral structure, suggesting it may be an irregular galaxy or a spiral galaxy undergoing tidal disruption. Overall the galaxy appears to be experiencing some form of morphological disturbance.
