The galaxy appears to be a relatively smooth, elliptical or lenticular type. Its overall shape is somewhat rounded, showing minimal distortion. There is a central concentration of light, suggesting a defined core or nucleus. The color profile indicates a predominantly older stellar population, as evidenced by the yellowish-red hue, suggesting lower ongoing star formation. No distinct spiral arms or bar structures are visible. There may be some evidence of a very minor disturbance in its overall structure, but it appears largely undisturbed.
