The galaxy presents as a somewhat elliptical, disk-shaped object. The central region exhibits a concentrated, bright yellowish-white luminosity, suggesting a substantial population of older stars and a possible supermassive black hole. Surrounding the core, there's a fainter, diffuse disk that appears slightly bluer in color, indicating the presence of younger, hotter stars and ongoing star formation activity. The galaxy does not exhibit any prominent spiral arm structures. There appear to be some minor irregularities in the outer disk, which could be due to tidal interactions, minor disturbances or possibly internal processes. Overall, the galaxy appears to be a relatively massive system with ongoing, moderate star formation. The morphology suggests a relatively evolved galaxy, potentially transitioning toward a more lenticular shape.
