The galaxy presents a relatively well-defined, although somewhat diffuse, disc structure. The overall color appears to be bluish, especially in the outer regions of the disc, indicating ongoing star formation. A brighter, more concentrated central bulge is evident, with a yellower hue suggestive of an older stellar population. There is a hint of spiral arm structure, but it is not highly pronounced or well-defined, and there is a suggestion of some asymmetry or disturbance in the overall structure. The galaxy shows signs of potentially being in interaction with another object. 
