The galaxy presents as a relatively smooth, centrally concentrated light distribution. It has an elliptical appearance, with the central region displaying a yellowish hue, indicative of an older stellar population. There's a slight gradient in color from the center outwards, with the outer regions appearing marginally bluer, suggesting the presence of some younger stars, though the overall population seems dominated by older stars. The light distribution is largely undisturbed, lacking any prominent spiral arms or tidal features, and is well-defined, with no visible signs of a major ongoing merger. The overall morphology suggests a evolved system that is not currently experiencing a high rate of star formation. 
