The galaxy presents a flattened, disk-like morphology. The central region exhibits a bright, concentrated core. Moving outwards from the core, there is a defined disk structure. The colors suggest the presence of both older stellar populations in the central bulge, indicated by the redder hues, and younger, hotter stars in the disk, represented by bluer tones. 

There is evidence of some disturbed features or asymmetries within the disk, perhaps indicating an ongoing or recent interaction with another galaxy. While a large portion of this object appears to be mostly undisturbed, a small portion appears to have a major disturbance to its profile, while the remaining portion has minor disturbances.
