The galaxy presents as a tilted, disk-shaped system. It is elongated, with a bright, concentrated central bulge that appears yellowish in color, potentially indicating an older stellar population. The disk exhibits a bluer hue, suggesting the presence of younger, hotter stars and regions of ongoing star formation. The galaxy does not display well-defined spiral arms, but there's evidence of some structural asymmetry or minor disturbances within the disk, particularly in terms of color variations and subtle lopsidedness. The outer regions of the disk fade gradually, with a noticeable dust lane or obscuration effect on the outer layers. Overall, the galaxy appears to be a moderately massive, actively star-forming disk galaxy at an intermediate redshift.
