The galaxy presents as a moderately inclined disk galaxy. It exhibits a prominent central bulge, characterized by a yellowish hue, which is indicative of an older stellar population. The surrounding disk displays a bluer color, suggesting the presence of ongoing star formation within the spiral arms. The spiral arms are not sharply defined, appearing somewhat diffuse. The overall shape of the galaxy appears to be somewhere between round and elongated. There are some slight disturbances in the galaxy, but no clear indication of a major merger.
