The galaxy appears to be relatively compact and centrally concentrated. It exhibits a generally smooth morphology, with no obvious spiral arm structure or prominent dust lanes visible in this image. The primary color of the galactic core is cyan, suggesting a population of young, hot stars or significant ongoing star formation in the central region. There is a more extended halo surrounding the core, exhibiting a slightly redder hue, which may indicate an older stellar population or the presence of dust absorption. There is a marginal degree of asymmetry in the shape and intensity distribution of the galaxy, but the galaxy itself is not visibly merging, although there may be minor disturbances. The galaxy is relatively isolated.