The galaxy presents a disk-like morphology with an approximate radius of 3 arcseconds. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant stellar density, potentially indicating the presence of a bulge. Moving outwards from the center, there is a noticeable decrease in luminosity. A faint and somewhat fragmented ring-like structure surrounds the central region. This ring appears bluer in color than the central region, potentially indicating the presence of younger stellar populations or regions of active star formation. There is a hint of minor disturbance, suggesting a possible ongoing interaction or recent merger event. Overall, the galaxy appears relatively smooth, with no obvious spiral arm structure or large-scale distortions.
