The galaxy appears to be a spiral type, though the arms are not particularly well-defined. There is a noticeable bulge in the center which appears to be moderately sized. The disk of the galaxy appears to be oriented at an angle with respect to our line of sight, it is not an edge-on galaxy. There may be a bar structure present, but this is not very obvious, and it is difficult to determine how strong the bar may be. There is a possible merger or interaction with a smaller galaxy, it could be experiencing some disturbance due to this interaction. The color distribution suggests ongoing star formation activity in the disk. The galaxy exhibits a generally smooth appearance, with subtle features in the spiral arms.
