This galaxy exhibits an elongated, cigar-like morphology. A central bulge is not clearly defined, indicating that the light is smoothly distributed. The color gradient suggests a potential difference in stellar populations across the galaxy, where regions closer to the central band are redder and the outer edges are bluer. This could indicate active star formation in the outer regions. The galaxy appears relatively undisturbed, and not to be a major merger. It seems there may be minor disturbances or distortions within its structure. This galaxy may be a low mass galaxy with ongoing star formation. 
