The galaxy presents a somewhat amorphous morphology, appearing neither strictly elliptical nor a well-defined spiral. There is a suggestion of a central bulge, with light appearing concentrated towards the center. However, the distribution of light is not perfectly smooth. Faint wisps or diffuse features extend outwards from the central region, indicating possible disturbances or interactions. 

There appears to be a slight blue shift in color in certain regions, possibly indicating areas of active star formation. Overall, the galaxy seems to be undergoing some sort of mild disruption, based on its irregular shape and the wispy features.
