The galaxy presents as a spiral type, viewed at a moderate inclination relative to our line of sight. A central bulge is readily apparent, with a yellowish hue, possibly indicating an older stellar population and reduced ongoing star formation in this region. A bar structure is discernable, appearing as a linear concentration of light across the galactic nucleus. The spiral arms are well-defined, and can be easily seen trailing outward from the ends of the bar. The arms themselves have a mottled appearance, likely indicative of regions of active star formation. There is a relatively smooth disk component. There is no evidence of significant tidal features or ongoing mergers. The overall morphology suggests a relatively undisturbed spiral galaxy.