The galaxy presents as a moderately bright object with a slightly elongated morphology. The primary body of the galaxy exhibits a smooth, concentrated appearance, suggesting a high degree of central mass concentration. There is a noticeable asymmetry in the overall structure, possibly indicating a disturbance or interaction with another galaxy. A distinct secondary component is observed, positioned close to the primary body, potentially representing a smaller galaxy in the process of merging, or tidal debris. The color profile is primarily reddish-yellow, implying an older stellar population with ongoing star formation. Evidence of disturbed morphology is present.
