The galaxy presents as a moderately luminous, elongated system. Its overall form appears relatively smooth, lacking prominent spiral arms or a large, obvious central bulge. The light distribution suggests a somewhat flattened shape, possibly indicative of an elliptical galaxy viewed at an oblique angle or a lenticular galaxy. There is a subtle color gradient across the galaxy's body, transitioning from slightly bluer hues on one side to redder hues on the other. This asymmetry in color could be attributed to variations in stellar populations and/or dust content across the galaxy. There is a suggestion of minor tidal disturbance, but its overall morphology is mostly undisturbed. The light is relatively concentrated, suggesting it could be fairly massive. Its observed color suggests it is actively forming new stars.
