The galaxy presents an elongated, cigar-like morphology. Its central bulge appears relatively smooth and bright, exhibiting a yellowish-white color, suggesting an older stellar population. Fainter, bluish hues are observed towards the outer regions of the galaxy. There is a slight indication of a disk structure, but it appears predominantly smooth with no clearly resolved spiral arm features. Minor disturbances are subtly visible, indicating a possibility for recent or ongoing interaction, although a major merger does not seem likely. The overall light distribution suggests a spectral energy distribution that peaks in the redder wavelengths, consistent with a moderate redshift. Considering the color and morphology, the galaxy exhibits characteristics consistent with a relatively massive system undergoing moderate levels of star formation.
