The galaxy presents as an elongated, disk-like structure, viewed at a high inclination. The central region appears brighter and more concentrated, indicative of a possible bulge or a higher density of stars. The outer regions of the disk exhibit a bluer hue, suggesting the presence of younger stellar populations and ongoing star formation. Overall, there is a relatively smooth appearance, with a slight hint of disturbances. The galaxy's light suggests a population of stars that are middle aged, but slightly more on the older end.