The galaxy presents as a slightly inclined disk galaxy. Its morphology reveals a central bulge region that appears smooth and concentrated. The disk component is visible extending outwards from the bulge. A faint spiral arm structure appears to be present, though not sharply defined. There is a slight asymmetry in the overall shape of the disk, which could be due to interactions or internal processes. The color gradient indicates that the central bulge likely consists of an older stellar population, with the disk showing bluer hues suggesting the presence of younger stars.
