The galaxy appears as a relatively small, somewhat diffuse object. There's a central concentration of light suggesting a nucleus or bulge, with fainter, irregular extensions radiating outwards. There is no clear spiral arm structure, and the galaxy appears flocculent.

The color is complex, with reddish tones concentrated towards the central region, and a greenish tinge in the outer regions. This color variation could be due to variations in the stellar population or dust content across the galaxy. The redder regions might be indicative of older, cooler stars, while the greenish hue may suggest the presence of ionized gas or younger stellar populations.
 
The overall morphology suggests a galaxy that has experienced some form of disturbance or interaction. The faint extensions are not organized into a regular disk-like structure. There are no signs of a large-scale merger, but there is a possibility of minor disturbances.
