The galaxy presents as a somewhat elongated, luminous structure. The central region exhibits a high degree of luminosity, appearing smooth and concentrated. Moving outwards from the center, the light gradually fades, blending into the surrounding space. The color profile suggests a mature stellar population, indicated by a yellowish-red hue, particularly prominent in the central bulge. The outer regions appear bluer, possibly indicating pockets of younger, hotter stars. Overall, the galaxy appears relatively undisturbed, lacking significant signs of ongoing mergers or tidal interactions. There is faint evidence of a disk-like structure, however, it presents more like a bulge-dominant system. There are no clear spiral arms or prominent dust lanes visible in this image.