The galaxy presents as an elongated structure, displaying a smooth, but not perfectly circular, morphology. A subtle color gradient is observed, with the central region exhibiting a more reddish-orange hue, suggestive of an older stellar population or significant dust obscuration. The outer regions of the galaxy appear to have a slightly bluer tint, which may indicate the presence of younger stars. There are no well-defined spiral arms or a prominent central bulge that can be clearly identified from this image. The overall structure suggests a possible elliptical morphology.
