The galaxy presents as a generally smooth, elongated structure. Its color appears to be predominantly yellow-orange, suggestive of an older stellar population. There is a slight color gradient observed, with the central region appearing more intensely yellow. The overall form is cigar-shaped, with no distinct spiral arm features discernable at this resolution. The edges of the galaxy appear somewhat diffuse, indicating a gradual decrease in stellar density. There is no obvious evidence of a strong central bulge or a distinct disk component.
