The galaxy presents as a moderately bright, centrally concentrated object. Its overall shape is elliptical, appearing nearly circular. The core region exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer outskirts are possibly visible, but the galaxy generally lacks significant features. The galaxy does not appear to be undergoing any major merging activity, but there is an indication of possible minor disturbance within the shape and structure. The galaxy's light is smoothly distributed, and there are no distinct spiral arms or bar structures observed.
