The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be generally elliptical, with a high degree of central condensation. The light distribution is somewhat diffuse, without any sharply defined features or spiral arm structures readily discernible in this imaging. A slight elongation is possibly present, although it is not significant. There is no evidence of any major merging activity. The galaxy exhibits a color gradient, appearing bluer towards its outer edges and more yellowish-orange towards the center.
