The galaxy presents as an elongated, disk-like structure, viewed at a significant inclination. The central region appears more concentrated and exhibits a yellowish-white hue, possibly indicating an older stellar population. Progressing outwards from the center, the disk displays a bluer color gradient, suggesting the presence of younger stars and regions of ongoing star formation. The disk appears relatively smooth, but may have some faint patches of brighter regions throughout. The galaxy does not display any prominent spiral arm structure or a well-defined bulge. Overall, it is a moderately sized, relatively low redshift system exhibiting a degree of flattening.
