The galaxy presents a generally smooth, rounded morphology. The light distribution appears centrally concentrated with a bright core, suggesting a significant bulge component. There is a gradual fading of light intensity from the core outwards. There is a slight greenish halo around the main body of the galaxy, suggesting the presence of some on-going, although subdued, star formation. There are no obvious spiral arms or a distinct disk component visible. Based on this, the galaxy appears to be an elliptical galaxy. There is no evidence of any major merger events, close tidal interactions, or strong disturbances in its structure. Overall, the system appears relatively quiescent.
