The galaxy exhibits a primarily disk-like morphology, appearing somewhat flattened. A bright, concentrated central region is evident, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outwards from the core, the disk presents a mottled texture suggesting the presence of star forming regions. 

The disk structure itself appears disturbed, lacking a clear spiral arm structure or a well-defined symmetrical shape. A minor interaction or tidal disturbance may be causing this asymmetric morphology. There is a presence of some color variation within the disk, with bluer tones suggesting regions of younger stars and active star formation and redder regions possibly containing older populations of stars. A faint halo may extend beyond the primary disk, but due to the image quality, this is difficult to ascertain with certainty. 
