The galaxy presents a flattened disk-like structure, viewed at an angle that is close to face-on. A central bulge region is discernible, appearing bright and concentrated, suggesting a high density of older stellar populations. Faint, diffuse spiral arm structures emanate from the central region, exhibiting a patchy distribution. These arms display bluish hues, indicative of ongoing star formation. The galaxy is located at a non-negligible distance, as determined by its measured redshift. The overall color profile suggests moderate recent star formation, contributing to an estimated mass. Interactions or recent mergers are not evident. The estimated size suggests a spiral galaxy of moderate proportions. The galaxy lacks any obvious signs of strong tidal distortion or active galactic nucleus activity.
