This galaxy exhibits a moderate angular size on the image. The galaxy appears to have a disturbed morphology, possibly indicating an ongoing interaction or recent merger event. We observe evidence of a tidal tail extending from the main body of the galaxy on one side. This feature presents as a fainter, elongated structure. Within the central region of the galaxy, there appears to be a concentration of older stellar populations. The color of these stellar populations trend towards a redder hue relative to the outer regions of the galaxy. Patches of bluer light can be seen in other areas, likely indicating the presence of younger stars or regions of active star formation. Overall, the galaxy presents a complex structure, suggesting a rich history of interactions.
