The galaxy presents as a diffuse, somewhat irregular structure. It is relatively compact in appearance, and the light distribution appears uneven, suggesting morphological disturbances. The galaxy exhibits a reddish hue, which could indicate an older stellar population or significant dust obscuration. There is a possible indication of minor tidal features, but not a clear, well-defined spiral arm structure. Overall, this appears to be a galaxy undergoing some form of interaction or disturbance.
