This galaxy exhibits a distinctly elongated, cigar-shaped morphology. Its light is primarily bluish in hue, potentially indicative of active star formation regions. The galaxy appears relatively smooth in texture, with minimal visible substructure such as spiral arms or prominent dust lanes. There are no readily apparent signs of a major ongoing merger, although there is perhaps some minor disturbance or asymmetry in the galaxy's outer regions that could be related to an interaction. The light seems brighter in the middle, and then evenly diffuses outwards. The small area it occupies and its overall smoothness lead me to believe this galaxy is relatively small and a low-mass system.
