The galaxy presents a predominantly bluish hue, suggesting the presence of younger stellar populations and ongoing star formation. Its morphology appears largely disturbed, lacking the clear spiral arm structure of a well-defined disk galaxy. Instead, the light distribution is somewhat irregular and clumpy, with a more concentrated, brighter region near the center that could represent a bulge or a region of intense star formation. Evident are hints of possible tidal features, potentially indicating past or ongoing merger activity with another galactic system. These disturbances are significant and may be driving an elevated rate of star formation within the galaxy.
