The galaxy presents as a spiral galaxy, moderately inclined to our line of sight. A prominent central bulge is observed, with a concentrated, bright luminosity. Distinct spiral arms emanate from the central region, exhibiting a somewhat loose winding pattern. These arms show clumpy regions suggestive of active star formation. The overall color of the galaxy indicates a mix of stellar populations, with the bulge appearing yellower, potentially indicative of older stars, while the spiral arms display bluer hues that are suggestive of younger, hotter stars. There is a hint of a bar-like structure spanning the center of the galaxy. The dust lanes and gas content are clearly visible in the arms.
