The galaxy presents as a slightly irregular, but generally smooth, luminous concentration. Its overall morphology does not strongly indicate a spiral disk structure; instead, it appears more spheroidal or elliptical in nature. Patches of redder hue suggest regions of older stellar populations or dust obscuration, while the bluish component indicates the presence of younger, hotter stars or ongoing star formation. Given the relative brightness and color indices, this galaxy may be experiencing moderate levels of star formation. There is some slight, but inconclusive, asymmetry in its morphology; there may be some type of minor interaction occurring.
