The galaxy presents a somewhat amorphous morphology. The central region displays a concentration of light, appearing relatively smooth and slightly elongated. Emanating from this central region are fainter, more diffuse structures that extend outwards, hinting at possible spiral arms or tidal features. These features lack sharp definition and appear somewhat disrupted, potentially indicating past interactions or ongoing disturbances within the galaxy. The overall color composition suggests a mix of stellar populations, with bluer hues visible in some of the outer regions, possibly indicating younger star formation, and yellower colors concentrated in the central bulge. Given the size and apparent luminosity, it could be a smaller galaxy of relatively low mass. The galaxy is somewhat faint and may have a low rate of star formation.
