The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology with high degree of roundness. A central bulge is observed, showing a concentration of light. The galaxy has an overall reddish-yellow hue, suggesting a population of older stars. There is very little evidence of spiral arm structure or significant dust lanes, with a smooth transition from the core to its edges. No obvious signs of major interactions or tidal features are present. The galaxy is compact, with a seemingly even light distribution. The galaxy is generally isolated in this image, showing no signs of a recent merger.
