The galaxy appears to be a disk galaxy seen at an oblique angle, approaching edge-on orientation. There is evidence of a bulge or central concentration of light, potentially indicating a supermassive black hole. The disk appears relatively smooth, which suggests a low ongoing star formation rate. However, the presence of some irregularities indicates a possible interaction. The galaxy has an absolute magnitude that suggests that it is a relatively luminous galaxy. Based on its morphology, a significant proportion of users have classified it as being an edge-on disk. A non-negligible fraction also believe it to be a merger, which is consistent with the interaction.
