The galaxy presents as a spiral type, with a relatively bright and concentrated central bulge. The bulge exhibits a yellow-white hue, indicative of an older stellar population. Spiral arms are present, though they are loosely wound and somewhat indistinct, extending from the central region. The arms show a patchy distribution of star formation. The galaxy displays a moderate inclination, allowing for a partial view of the galactic disk. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The colors of the disc and spiral arms hint at a varied stellar population, with some regions possibly exhibiting ongoing star formation.
