The galaxy appears as a moderately sized, centrally concentrated object. It exhibits a relatively smooth, diffuse light distribution, lacking prominent spiral arms or a distinct bar structure. The color profile suggests a slightly redder hue, potentially indicating an older stellar population or significant dust obscuration. There is no clear evidence of a recent major merger event; however, there may be some subtle distortions in the outer regions, possibly indicating minor gravitational interactions. The general morphology is consistent with an elliptical galaxy, or possibly a lenticular galaxy viewed at a shallow inclination.
