The galaxy presents as a centrally concentrated object with a moderate degree of radial symmetry. Its light profile appears largely smooth, indicating a likely classification of elliptical or lenticular. The core region exhibits a yellowish-white hue, suggesting an older stellar population. There are minor asymmetries on the left side and hint of bluer light. There is no distinct spiral arm structure visible; the overall form is fairly uniform and rounded. Given the lack of any significant tidal tails or distortions, there is no indication of recent major merger activity. Overall, the galaxy appears to be relatively undisturbed.
