The galaxy presents an elongated, cigar-like morphology. It exhibits a smooth, diffuse profile with no readily discernible spiral arms or distinct features. The central region appears to have a higher concentration of light, suggesting a central bulge. The color is generally yellowish-orange, possibly indicating an older stellar population, with hints of blue particularly in the outer regions, suggestive of some ongoing star formation. There is no obvious evidence of a recent major merger or significant tidal disruption. The system appears to be relatively isolated and undisturbed.
