The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears centrally bright and gradually fades towards the outer regions, suggesting an older stellar population. The color indices indicate a redder hue overall with tinges of green, typical of galaxies where star formation has slowed or ceased, with a likely prominence of older, redder stars. The object exhibits a fairly high degree of symmetry and no distinct spiral arm structure is discernible within the limits of the resolution. No tidal features or other signs of ongoing or recent major merger events are obvious, though there might be minor disturbances. The object's color is dominated by a yellowish hue in the central region.
