This galaxy presents as a flattened, disk-like structure with a bright, concentrated central bulge. There is a definite red shift in the overall color distribution, which is more prominent along the edges of the galaxy. This is contrasted by a brighter central region appearing more yellow and white. The overall texture appears smooth, with no immediately obvious spiral arm structures. A distinct blue emission is visible. This may indicate a region of active star formation, or could be due to interaction with something external. There is slight asymmetry in the disk which may suggest a minor disturbance. However, given the overall smooth appearance, interaction is unlikely to result in major disruption of the galaxy's structure. There are no obvious signs of a major merger event.
