The object presents as a galaxy exhibiting a disturbed morphology, likely undergoing a merger or interaction with another galaxy. There is a primary, more luminous component that appears relatively smooth but with an elongated shape. Emanating from this central region are tidal features or plumes, indicative of gravitational disruption. The color profile suggests a mix of stellar populations, with reddish hues possibly indicating older stars or dust obscuration, while the brighter, yellowish regions may signify ongoing star formation. Overall, the galaxy appears to be in a dynamically active state.
