The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with high degree of roundness. There is a lack of distinct spiral arm structures or prominent dust lanes visible in this image. The central region shows a brighter, more intense yellow color, potentially indicating an older stellar population. Fainter, diffuse outer regions extend outwards from the central core, surrounded by a slight halo-like distribution of light. No obvious signs of ongoing major mergers or strong tidal disturbances are apparent. Overall, the galaxy appears to be a relatively evolved system with a dominant smooth component.
