The galaxy presents as an edge-on or highly inclined disk galaxy. The central bulge appears prominent and exhibits a concentrated, yellowish-orange hue, possibly indicative of an older stellar population. A relatively faint and diffuse disk extends outward from the bulge, displaying a somewhat irregular structure. There is a subtle hint of asymmetry in the disk's morphology. The disk displays bluer regions which are indicative of younger stars and ongoing star formation. The overall color suggests a mix of stellar populations. There is little evidence of strong spiral arm structure. There is an appearance of minor disruption or disturbance, based on slight asymmetry and irregular features.
