The galaxy presents a generally smooth morphology, suggesting a predominantly evolved stellar population. The color gradient exhibits a shift from a redder hue at the galactic center, which gradually fades to a more greenish-blue periphery. This color difference might be due to the central bulge being comprised of older stars as opposed to younger stars on the outskirts. There appears to be little to no spiral arm structure, which is consistent with the smooth appearance of the galaxy. The galaxy is also significantly elongated. The edge-on orientation obscures a more detailed examination of the inner structure, such as a central bulge or the presence of a bar. There is no obvious presence of a dust lane. The galaxy does not appear to be undergoing a major merging event.
