The galaxy appears as a relatively small, faint object with a somewhat elongated, cigar-like morphology. It exhibits a generally smooth profile, lacking any prominent spiral arms or significant knots of star formation that would suggest a disk structure. The light is fairly uniform across the body of the galaxy, with a subtle central concentration. The color is predominantly bluish, hinting at a population of somewhat younger stars relative to older, redder stellar populations. There is no visual indication of any ongoing major merger activity or significant tidal disturbances. The apparent lack of fine detail suggests that this is a distant galaxy, and we are observing the integrated light from its stellar population. The galaxy is likely a low-mass system with a low rate of star formation.
