The galaxy presents as a system undergoing a significant interaction or merger. The primary body exhibits a disturbed morphology, lacking a clear spiral or elliptical structure. A brighter central region is visible, surrounded by a less defined, extended halo or disk. Two distinct luminous clumps or tidal tails are apparent. The upper clump exhibits a bluer hue, suggestive of ongoing star formation. The lower clump is closer to the main body and displays a yellower hue. The overall color profile suggests a mix of stellar populations, with evidence of both older, redder stars and younger, bluer stars. Tidal features and distortions indicate strong gravitational forces at play, likely due to an ongoing or recent merger event. The estimated size of the galaxy is on the order of 6.6 kpc, suggesting a moderately sized system.
