The galaxy presents a somewhat elliptical morphology, with a distinct central bulge. It appears to be a spiral galaxy, however, the arms are tightly wound around the central bulge, making them difficult to discern. The bulge dominates the galaxy's overall luminosity. There may be a weak bar feature present across the center of the bulge, but is is hard to be certain. The galaxy's light profile suggests moderate recent star formation, particularly in its spiral arms if they exist, in addition to the older stellar population contributing to the bulge's light. The light in the spiral arms appears to be fairly uniform in color, suggesting that it may not be actively forming stars at a large rate. The overall color gradient moves from yellow in the center to white at the edges. The center may have more light from older, redder stars whereas the white color shows that the outer sections of the galaxy may have more newer, bluer stars. It doesn't appear to be undergoing any major merging activity, but there could be some minor disturbances.
