The galaxy presents as a moderately faint, relatively small object. It appears elliptical in shape, showing a smooth, diffuse distribution of light without prominent spiral arms or a distinct central bulge. The color appears somewhat uniform across the galaxy, suggesting an older stellar population with lower rates of star formation. There is no visual evidence of ongoing major mergers or tidal disturbances, though minor irregularities in the overall light distribution cannot be ruled out. Based on its morphology, the galaxy is likely an early-type galaxy with a mass around 10^10 solar masses.
