The galaxy appears as a moderately bright, elongated object with a generally smooth morphology. Its color profile suggests a concentration of older stellar populations, giving it a yellowish-orange hue. There is a slight suggestion of a disk-like structure, although the overall light distribution is fairly uniform. The galaxy does not show any prominent signs of active star formation or major disturbances. Its shape is more elongated than circular, with a hint of a cigar-like appearance. There's no obvious evidence of ongoing mergers or tidal interactions, indicating that it has likely been relatively undisturbed recently. Overall, it appears to be a relatively evolved galaxy with a passive star-formation history.
