The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing largely spheroidal in shape. The central region displays a yellow-orange hue, potentially indicative of an older stellar population. Surrounding this core, there is a discernible blue halo, suggesting the presence of younger, hotter stars, or ongoing star formation, at a lower rate relative to its overall mass. There is no clear indication of spiral arms or a well-defined disk structure in this image. The galaxy appears relatively isolated, with no obvious signs of tidal disturbances or major interactions with other galaxies.
