This galaxy exhibits a morphology suggesting a recent or ongoing interaction. The primary body of the galaxy appears roughly spherical, with a central concentration of light. There is evidence of a tidal tail extending from the main body. The tail shows a gradient in color, shifting from bluer tones near the main body to redder tones further away. This might suggest a difference in stellar population, where bluer, younger stars closer to the galaxy are from a recent burst of star formation triggered by the interaction and redder, older stars are further away. The main body of the galaxy displays a greenish hue, which might indicate the presence of ionized gas or a mix of stellar populations. The object appears relatively compact, but detailed spectroscopic analysis would be necessary to determine its redshift, internal kinematics, and the composition of its stellar populations. It could be that the morphology is due to a minor merger or gravitational interaction.
