The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, lacking prominent spiral arms or distinct features within its structure. The central region of the galaxy exhibits a yellowish hue, possibly indicating an older stellar population or dust obscuration. Fainter blueish tinges can be seen at the edges of the galaxy. The galaxy displays signs of potential tidal disturbance or interaction based on it's irregular shape. There's no strong evidence of on-going, high levels of star formation.
