The galaxy presents as a single, elongated object. Its light profile is dominated by redder wavelengths, suggestive of an older stellar population, however, a slight gradient towards bluer hues near the apparent center could indicate ongoing star formation, albeit at a modest rate. The galaxy appears mostly smooth, with a noticeable cigar-like shape. There is no strong evidence of a bulge or disk structure from what is visible in this image. There is no apparent interaction with nearby galaxies.