The galaxy presents with a centrally concentrated luminosity profile, appearing roughly circular in shape, with an estimated radius of about 4.5 arcseconds. The central region exhibits a bright, smooth, and largely featureless appearance, suggesting a dominant spheroid component. While a distinct disk structure is not readily apparent, subtle color variations hint at the possibility of underlying structures. The colors are consistent across the galaxy. There are no obvious signs of tidal tails, merging features, or other major disturbances, however subtle irregularities near the galaxy's periphery cannot be ruled out due to image resolution. 
