The galaxy presents an elliptical morphology, characterized by a centrally concentrated spheroid component. The color gradient suggests an older stellar population dominating the core, evidenced by the yellowish hue. Moving outwards, the galaxy exhibits a bluer color, possibly indicating the presence of younger stars and ongoing star formation within the galaxy's extended disk. There appear to be some minor disturbances within the galaxy, the disturbances could potentially arise from tidal interactions or past minor merger events, although a more detailed spectral analysis would be required to confirm the presence of these disturbances. Overall, the galaxy appears to be an intermediate mass system with relatively low ongoing star formation. 
