The galaxy presents as a luminous, elongated structure with a distinct central bulge. Its morphology suggests a potential disk galaxy viewed at an inclined angle. There is a noticeable color gradient, with the central bulge appearing more yellow or golden in hue, potentially indicating an older stellar population. Fainter, bluish extensions emanate from the main body, possibly indicating regions of more recent star formation. The overall appearance exhibits signs of tidal disruption or interaction, evidenced by the asymmetric shape and faint extensions, suggesting a possible ongoing or recent merger event. It is worth further investigating the spectral properties to confirm the age of stellar populations and the rate of star formation, as well as, analyze its surrounding environment for further signs of interaction.
