The galaxy presents an elliptical morphology with evidence of a disk component. There appears to be a central bulge exhibiting a yellowish hue, with the disk demonstrating a bluer color profile overall, suggesting ongoing star formation. Faint spiral arm structures can be discerned within the disk. The galaxy exhibits a slight tilt, as it is not perfectly face-on. There is also a region of bright red light that is visibly separated from the main body of the galaxy and to the left of the main body, and another similar but much smaller red formation to the lower central region of the image that seems to be a part of the galactic structure. These regions likely represent areas of intense star formation or other emission phenomena.
