The galaxy presents as a slightly disturbed spiral form at redshift z ~ 0.2. Its apparent magnitude suggests a luminous galaxy. The central bulge appears relatively indistinct, with some evidence of diffuse emission. There are hints of spiral arm structure, albeit somewhat disrupted, indicated by subtle variations in color and density. A very minor disturbance is visible in the galaxy's features, indicating a possibility of a past merger event or ongoing gravitational interactions with a nearby companion, though no companion object is obvious in the immediate vicinity. Star formation appears to be ongoing, evidenced by the presence of some blue regions within the spiral arms. A rough estimation suggests a stellar mass on the order of 10^9 solar masses. The specific star formation rate appears somewhat suppressed.
