The galaxy appears to be a relatively compact object, exhibiting a moderately bright core. There is some suggestion of a disk-like structure surrounding the central region, though it is not sharply defined. A faint halo or extended emission surrounds the brighter inner regions. The object's color profile indicates a blue tint overall, with a slightly redder periphery. Some irregularities in the brightness distribution indicate possible minor disturbances or ongoing interactions. It appears to be a spiral galaxy with some level of disturbance. 
