The observed galaxy presents as a moderately redshifted system. Morphologically, it appears as an elongated, cigar-shaped object with a relatively smooth profile. The galaxy exhibits a distinct color gradient across its structure, transitioning from a redder hue at its central region towards bluer tones extending to its outermost edges. The galaxy disk appears to be at a high inclination with respect to our line of sight. There is no sign of active galactic nuclei or other galaxy interactions such as merging or tidal tails. Star formation appears to be more concentrated in the outer regions of the galaxy.
