The galaxy presents an overall irregular morphology. The central region exhibits a bright, concentrated luminosity, appearing somewhat smooth in texture. However, this smooth core is surrounded by more diffuse and less organized structures. There appear to be faint hints of tidal features or disrupted spiral arms, suggesting possible past or ongoing gravitational interactions. The color distribution is complex, with the central region displaying a bluer hue indicative of younger stellar populations, while the outer regions show redder tones, suggesting older stars and dust. There may be a merger occurring, or a recent occurrence, as minor disturbances are apparent within the features of the galaxy. The galaxy does not appear to be spheroidal.