The galaxy presents as a moderately bright, disk-shaped object. The disk is noticeably tilted relative to our line of sight, appearing elongated rather than circular. The color distribution is not uniform across the galaxy. A brighter, slightly redder core is evident, indicative of a higher concentration of older stellar populations and dust. The outer regions of the disk appear bluer, suggesting ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. There might be some minor disturbances in the outer regions. The galaxy exhibits an estimated diameter of approximately 5 kpc and appears to be at a distance where its redshift is measured to be approximately 0.23. Given this redshift, this galaxy demonstrates moderate mass and star formation rate.
