The observed galaxy presents a morphology indicative of a spiral structure, displaying prominent, well-defined spiral arms. These arms exhibit a predominantly medium winding pattern. Two spiral arms appear to extend from a moderate-sized central bulge, which appears to be composed of an older stellar population. Evident are signs of potential interaction, displaying significant disturbances in the galaxy's overall structure, potentially indicative of an ongoing or recent merger event. The disk is generally face-on. This galaxy exhibits a blue hue in its spiral arms suggesting more recent star formation. The galaxy has a redshift measurement, indicating its distance.
