The observed galaxy presents a somewhat disturbed morphology. The primary body appears relatively smooth but exhibits a distinct asymmetry in its overall form. A faint tidal tail is visible, suggesting a gravitational interaction or recent merger event. The galaxy's color gradient indicates a higher concentration of younger, bluer stars in the outer regions and relatively older, redder stars towards the core, although these features are not very distinguishable and are generally more homogenous. Faint spiral arm structures are potentially present but are not well defined, adding to the ambiguity of its overall structure. The galaxy appears to be undergoing some degree of disruption or merging based on the slight irregularities and color distribution present. The core itself appears relatively compact. Overall, the galaxy displays characteristics indicative of a system experiencing tidal forces, potentially due to a minor ongoing or past merger. 
