The galaxy exhibits a somewhat elliptical morphology, appearing as a flattened spheroid. The light distribution suggests a smooth profile, with a high degree of central concentration. There is no discernible spiral arm structure, but the outer regions do seem to fade gradually into the background. The core is a relatively brighter and more compact region, with the color distribution indicating the presence of older stellar populations throughout the entirety of the galaxy. The galaxy shows no evidence of significant dust lanes or patchy star formation regions within the limitations of this image. Overall, the galaxy appears to be a relatively quiescent system.
