This galaxy exhibits a disk-like morphology, although it is not perfectly face-on. The central bulge appears prominent, with a yellowish hue suggesting an older stellar population and less ongoing star formation in this region. The surrounding disk shows hints of blue, indicating younger, hotter stars and active star-forming regions, though this is not particularly pronounced. There is a suggestion of disturbed morphology, with the galaxy possibly undergoing an interaction or merger. This is based on the presence of faint tidal features or asymmetries in the outer regions of the galaxy. It seems there may be other galaxies near it. The color gradients within the galaxy suggest variations in stellar populations and dust content. Overall, it appears to be a relatively small to medium-sized galaxy with a complex evolutionary history, potentially shaped by past or ongoing interactions.
