The galaxy presents a somewhat elongated, though not perfectly elliptical, morphology. A central bulge region displays a yellowish-orange hue, suggestive of an older stellar population likely dominated by evolved red giant stars. Moving outward from the bulge, a faint, disklike structure is observed. This disk exhibits a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. 

Evidence of some disturbance within the galaxy is noted; the disk appears slightly asymmetrical or warped, rather than a uniformly flat plane, which may indicate a previous interaction with another galaxy. There appears to be no dominant spiral arm structure. The overall morphology is complex, falling somewhere on the spectrum between a spiral and an elliptical galaxy. It is neither clearly one or the other.
