The galaxy presents as a highly inclined, likely disk-shaped system. The dominant feature is the pronounced central bulge, which appears bright and yellowish, indicating a population of older stars. Fainter spiral arms are not clearly visible. The disk itself is relatively smooth in appearance, suggesting a well-mixed stellar population or significant dust obscuration. Given the inclination, it appears largely edge-on, with a potential for a boxy or rounded bulge morphology. There is no obvious evidence of ongoing major mergers or strong tidal disturbances. There is some indication of ongoing star formation. The overall color is redder than other galaxies, suggesting an older stellar population and lower levels of star formation.
