The galaxy presents as a relatively smooth, centrally concentrated object with an approximately elliptical morphology. There is a high degree of radial symmetry, with minimal evidence of spiral arm structure or significant irregularities. The color profile indicates a general blueness, implying the presence of a younger stellar population within the galaxy, although not extremely blue. No prominent dust lanes or signs of active galactic nuclei are clearly visible in this image, though it is likely very far away. Based on its appearance, this galaxy is a likely an elliptical galaxy. The galaxy does not appear to be undergoing any major merging events, though there are minor disturbances.
