The galaxy presents as a spiral galaxy, viewed at an oblique angle, but not quite edge-on. There's evidence of loosely wound spiral arms that extend from a bright central bulge. The arms are somewhat patchy in appearance, indicating regions of active star formation. The central bulge appears relatively smooth and featureless. There is a suggestion of some disturbance in the morphology of the disk, hinting at a possible minor interaction or merger in its past. The overall color suggests a mix of stellar populations, with some bluer regions in the spiral arms indicative of younger, hotter stars, and a yellower central bulge that contains an older stellar population.
