The galaxy appears as a central bulge with a flattened disk extending outwards. The core of the galaxy exhibits a brighter, more concentrated luminosity, potentially indicative of a supermassive black hole or a dense stellar population. The disk structure is subtly visible. The overall form of the galaxy appears to be disturbed. There is faint evidence of interaction with a small, close neighbour or the remnants of a recent merger. The galaxy exhibits a moderate redshift and a corresponding luminosity and stellar mass consistent with a typical large galaxy. Star formation appears relatively low, suggesting a passively evolving system. The disk displays a gradient in color, transitioning from yellower hues near the center to slightly bluer tones in the outer regions, possibly suggesting the presence of younger stars. The galaxy is not perfectly circular, indicating it may not be a face-on spiral galaxy.
