The galaxy presents an overall elliptical morphology, but with hints of a disturbed structure. There is a central bulge that appears relatively smooth and concentrated. Fainter, diffuse light surrounds the central bulge, extending outwards in a somewhat flattened disk-like structure. 

Within the disk, subtle irregularities and asymmetries are visible, potentially indicating tidal interactions or minor disturbances. The colors observed range from yellowish-white in the center to bluish hues in the outer regions, suggestive of varying stellar populations.

Given the evidence of potential interactions along with apparent ongoing star formation, this object is likely undergoing some form of evolutionary process, though the exact nature of this activity warrants further investigation.
