The galaxy exhibits a generally elliptical morphology, appearing somewhat flattened along its periphery. There is a central bulge that is relatively bright, and appears to have a high surface brightness. The outer regions of the galaxy show a fainter, disk-like structure, though ill-defined. There are some structural irregularities that seem to be small disturbances, or possible tidal effects. The galaxy appears to have a smooth overall texture, with a notable lack of defined spiral arms or prominent dust lanes. The color profile suggests a mix of stellar populations, with the central bulge possibly dominated by older, redder stars, and the outer disk exhibiting bluer colors indicative of younger stars, but with limited star formation. Overall, the galaxy may be undergoing some kind of interaction or minor merger.
