The galaxy exhibits a generally smooth morphology, with a somewhat elongated, cigar-shaped structure. A central bulge is present, appearing more concentrated and with a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint, potentially indicating the presence of younger stars and ongoing star formation, although the rate seems relatively low. There is no clear evidence of spiral arms or a well-defined disk, with the overall structure being rather amorphous. There are no obvious signs of a major ongoing merger or significant tidal disturbances, although there could be minor interactions occurring. The galaxy's light is redshifted, indicating it is at a considerable distance.
