The galaxy presents a disturbed morphology, potentially indicative of an ongoing or recent merger event. The central region exhibits a bright, concentrated core with a yellowish hue, suggesting a population of older stars. Extending outwards is a bluer, less defined region, showing the possible presence of younger stellar populations and ongoing star formation. The overall shape appears elongated, deviating significantly from a regular elliptical or spiral structure. Faint tidal features are suspected, hinting at gravitational interactions with another galaxy. The galaxy does not present a well-defined spiral arm structure, nor does it exhibit a smooth elliptical profile. 
