The galaxy presents an elongated, cigar-shaped morphology, indicative of a potentially elliptical or lenticular galaxy. It exhibits a smooth, diffuse appearance with a centrally concentrated luminosity profile that fades towards the outer edges. The galaxy's color profile suggests a higher concentration of older stellar populations, as evidenced by its redder hue towards the center with bluer hues in the surrounding disc. There are no prominent spiral arms or dust lanes visible. The overall light distribution is relatively uniform with a ratio of short to long axis around 0.43. Its size is roughly estimated to be 9.5 kpc in diameter. There is no noticeable strong interaction with neighboring galaxies or tidal streams. The redshift of the galaxy places it at a significant cosmological distance.