The galaxy presents an overall reddish hue, suggesting an older stellar population. A noticeable asymmetry is observed in its morphology. One side appears to exhibit a more extended, diffuse structure with a yellowish tint, which could indicate regions of recent star formation or tidal interactions. The central region presents a brighter, more compact core. There are hints of disturbed structure around the core which indicate that the galaxy might be in the process of merging with another galaxy. Some areas surrounding the galaxy indicate a merging of a close object. Overall, this is a galaxy with signs of interaction and potential ongoing disturbances.
