The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests a likely elliptical classification due to its high degree of roundness. The galaxy displays a radial color gradient, appearing bluer towards its core, which could indicate the presence of a younger stellar population or ongoing star formation in the central regions. There is no apparent disk structure or spiral arms. A lack of significant tidal features or morphological disturbances argues against recent major merger activity. Subtle irregularities may indicate minor interactions or internal processes. Overall, the galaxy appears to be a relatively evolved system. 
