The galaxy presents as a spiral type, viewed at an angle that suggests a primarily face-on orientation. It exhibits a bright, concentrated central bulge. Spiral arms are visible, branching outwards from the core region and exhibiting a somewhat flocculent structure. Evidence for active star formation is suggested by blue-ish tinges within the spiral arms. The color of the galaxy is bluish, indicative of a population of relatively young, hot stars. There is no indication of a major merger event or significant tidal disruption. A weak bar may be present bisecting the bulge.
