The galaxy presents an elongated, cigar-shaped morphology. The central bulge appears prominent and exhibits a smooth, relatively featureless structure with a concentrated bright core. The color suggests a population of older stars. Extending outwards from the central bulge is a fainter, less defined disk. The disk appears relatively smooth with a suggestion of some structure. There is a subtle color gradient from the center to the outer regions. The overall appearance indicates a system that is not currently undergoing significant merger activity.
