The galaxy presents as a system with a disturbed morphology. Its overall shape is elongated, approximately 6.5 kpc in radius, and deviates significantly from a regular elliptical or spiral form. The primary body displays a generally smooth appearance with an orange hue, suggesting a population of older stars. However, distinct features are observed in the form of brighter, less defined regions arranged along a curve that would indicate disturbed spiral arms were visible from this distance. The light coming from the "arms" shows a bluer shift, potentially indicating current or recent star formation. The morphology is not indicative of a late-stage merger but shows signs of minor tidal disturbance, possibly due to a previous interaction or ongoing accretion. The relatively high roundness and absence of a clear disk-like structure further suggest an intermediate morphological type, evolving from a spiral towards a more spheroidal configuration.
