The galaxy presents as a centrally concentrated, relatively smooth elliptical or lenticular system. The core region exhibits a yellowish-white color, potentially indicative of an older stellar population. Surrounding the core is a fainter, more diffuse halo extending outwards. This halo shows hints of a bluer hue compared to the central region, suggesting the presence of a younger stellar population or ongoing, albeit subdued, star formation activity. Overall, the galaxy appears to be largely undisturbed, with a regular, rounded morphology. No prominent spiral arms or significant dust lanes are discernible within the visible structure. The galaxy's light profile appears to decrease steadily from the core to the outer regions.
