The galaxy presents a flattened, disk-like morphology viewed at a moderate inclination. Evidence suggests it is mostly smooth in overall appearance but there is some subtle, low-contrast structure within the disk, possibly indicating faint spiral arms or patchy star formation regions. The color gradient from the center outwards is not very pronounced, it's more or less similar throughout the galaxy. There is no prominent bulge component visible, implying either a small bulge size, or that the bulge is obscured. There is no apparent tidal features suggesting it is not currently undergoing a major merger or strong gravitational interaction.
