The galaxy presents as a somewhat diffuse object with a slightly elongated morphology. Its light distribution suggests a central concentration of older stellar populations, characterized by a yellowish-red hue. Surrounding this core, a fainter, bluer component extends outwards, hinting at ongoing or recent star formation activity. The structure appears disturbed, possibly indicating an interaction or merger event. There are hints of irregular features or tidal tails extending from the main body, supporting the idea of gravitational disturbance. The overall appearance suggests a transitionary phase in its evolutionary history, possibly between a more regular spiral or elliptical form and a state of increased irregularity driven by external forces.