This galaxy presents as a somewhat elongated, diffuse object. Its central region exhibits a brighter luminosity, suggesting a higher concentration of stellar mass or active galactic nucleus activity. A slight extension or plume is visible to one side of the main body, hinting at a possible interaction with another galaxy or tidal distortion. The galaxy's overall structure appears relatively smooth, with a lack of distinct spiral arms or prominent features, possibly indicating an elliptical or lenticular morphology. The observed color profile suggests active star formation or a redshift in the z band. While the galaxy appears mostly undisturbed, there is slight asymmetry, suggesting a minor gravitational interaction.
