The galaxy presents a primarily smooth morphology. There is a bright central bulge region appearing roughly circular in shape. The color of the central region is predominantly bluish-white, suggesting the presence of a population of hot, young stars or active galactic nucleus activity. The surrounding disk is relatively faint. There are indications of faint, diffuse features extending outward from the central region, potentially indicating a minor disturbance or tidal interactions. The galaxy appears to be fairly compact in size. Faint, diffuse extensions might hint at ongoing or past mergers, or tidal streams. 
