This galaxy presents a complex morphological structure. The central region appears smooth and concentrated, suggesting a possible bulge component. Surrounding this bulge, there is a distinct, relatively bright disk. 

The galaxy exhibits a generally elliptical shape, with a noticeable flattening indicative of a rotating system. The color profile suggests a mix of stellar populations, with the central bulge exhibiting a slightly redder hue compared to the bluer disk. Evidence suggests a low level of ongoing star formation.

There appear to be some disturbances present within the disk, although not significant. 
