The galaxy presents an elongated, cigar-shaped morphology, potentially an elliptical galaxy viewed at an angle. The central region exhibits a bright, concentrated luminosity, indicating a high density of stars, while the outer regions appear fainter and more diffuse. A subtle blue hue permeates the galaxy's light, more concentrated in the center, which might suggest the presence of younger stars and ongoing, though subdued, star formation processes. No distinct spiral arms or dust lanes are discernible in this image. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or tidal interactions.