The galaxy presents as a relatively smooth, elliptical object. Its morphology appears largely undisturbed, with no obvious signs of a major merger event. The primary color is a yellow-orange hue, which suggests a stellar population dominated by older, redder stars, and relatively low ongoing star formation. There is a slight gradient in color, with the central region appearing somewhat more yellow than the outer regions. The roundness of the galaxy is rather high, which helps determine its type. Subtle irregularities might be present, but the resolution limits detailed analysis of faint features. There's a slight asymmetry in the light distribution which could suggest some ongoing minor interaction, however further investigation would be needed to confirm this hypothesis.
