The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology with a relatively round shape. There's a slight deviation from perfect circularity, indicating a possible intermediate ellipticity. No distinct spiral arm structures are visible, nor are any signs of strong tidal disturbances or ongoing major merger activity. There is a subtle suggestion of a minor disturbance within the galaxy's structure.

Based on its color indices, the galaxy exhibits moderate stellar population age with a blend of young and older stars, and there is ongoing star formation activity. 
