The galaxy presents as an elongated, cigar-shaped form. There is no distinct central bulge, suggesting it is either a late-type spiral seen edge-on or a lenticular galaxy with a very flattened disk. Its light profile appears relatively smooth and diffuse with no signs of prominent spiral arms or dust lanes visible in this image. The bluer hue of the galaxy suggests the presence of a modest population of young, hot stars, and the blue light is not highly concentrated in any particular region. There is no obvious sign of major mergers or tidal disturbances to the galaxy, although a minor interaction cannot be ruled out based solely on this image. Overall, the galaxy exhibits characteristics of an evolving system, displaying signs of low to moderate star formation activity without significant ongoing disruption.
