The galaxy presents as an elliptical or lenticular type, with a high degree of central concentration. A smooth, relatively featureless structure is evident throughout the galaxy body. The radial light profile appears to decline smoothly from the bright central region outwards, with no distinct spiral arms or bar-like structures observed. The galaxy exhibits a yellowish hue, suggesting a stellar population dominated by older, redder stars. There is a lack of observable blue light indicative of minimal ongoing star formation. The galaxy appears isolated, with no signs of major tidal distortions or interactions with nearby galaxies.
