This galaxy presents a distinctly elongated, cigar-like morphology. It appears primarily smooth in texture with no readily apparent spiral arm structure. The central bulge is a pale yellow or white hue, indicating a possible older stellar population. Moving outward from the central bulge, there is a subtle change to a bluish color, suggesting the presence of some younger stars within the disk. The galaxy appears relatively isolated, with no obvious signs of ongoing or recent major mergers. There may be a minor disturbance or interaction causing the slight asymmetric shape of the galaxy. The overall color profile suggests the galaxy may be transitioning from a period of higher star formation to a more quiescent state. The overall scale and luminosity indicate a relatively modest-sized galaxy at the observed redshift.
