The galaxy appears as a flattened, elliptical structure with a smooth, diffuse light distribution, suggesting a relatively old stellar population. The galaxy exhibits a cigar-like morphology, significantly longer along its major axis than its minor axis. There is no clear evidence of spiral arms or a central bulge. There is a slight color gradient across the galaxy, with the central region appearing more yellow in hue compared to its outskirts, implying the presence of older, redder stars concentrated in the center. No tidal features or signs of recent merger activity are readily apparent, though the galaxy's overall shape indicates it may have undergone a past interaction or minor disturbance. The galaxy's intermediate redshift indicates that it is a fairly distant object. Its relatively high mass and low star formation rate suggest a significant fraction of its gas has been consumed by the star formation.
