The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color profile exhibits a central concentration of yellow light, suggesting an older stellar population dominates the core. The light appears to gradually fade towards the outer regions of the galaxy. There is a faint but distinct bluish area on the lower left side of the main body. The overall shape is mostly round, with no immediately obvious signs of spiral arms or significant tidal distortions, but there are some slight irregularities in the luminosity distribution, indicating minor disturbances. The galaxy seems to be relatively isolated with a slight chance of merger.
