The galaxy appears as a relatively smooth, elongated structure. It exhibits a central, bright bulge region which fades gradually into the outer regions, and the overall color appears to be yellowish, especially in the central bulge, suggesting a relatively older stellar population. The outer disk exhibits subtle signs of structure, but lacks prominent spiral arms or strong features. The overall shape is moderately elongated, not quite cigar shaped, but not perfectly round either. There are no obvious signs of ongoing major mergers, although subtle disturbances cannot be ruled out.
