This galaxy presents as a somewhat diffuse, yet structured object. While a distinct spiral structure is not immediately apparent, there are hints of non-uniformity in the distribution of light, suggesting possible features or disturbances.

The galaxy appears to be undergoing some form of interaction or merger. The light distribution is not uniform, with some areas appearing brighter than others. The overall color is shifted slightly towards the redder end of the spectrum, especially when compared to the surrounding background. This could indicate an older stellar population. However, there are also patches of light visible, indicating possible areas of ongoing star formation. Overall the galaxy does not appear to be very smooth, and shows some degree of disturbance.
