The galaxy presents as a relatively smooth, centrally concentrated structure. It displays a slightly elliptical morphology, with no obvious spiral arm structures visible. The color profile indicates a generally older stellar population, with a yellowish hue dominating the core. There appears to be a subtle extension of diffuse light surrounding the central region, forming a faint halo. No prominent dust lanes or regions of intense star formation are immediately apparent in this image. Overall, the galaxy's morphology suggests an evolved system, potentially a lenticular or early-type spiral galaxy viewed at a considerable distance.
