The galaxy presents an elliptical morphology, appearing largely smooth in structure with no prominent spiral arms or bar features visible. The central bulge region appears bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population dominates this area. Extending outwards from the core, the galaxy displays a more diffuse, fainter halo. This halo demonstrates subtle variations in color, with hints of bluer regions, possibly indicative of younger, hotter stars or ongoing star formation in the outer regions. Overall, the galaxy appears to be at an intermediate inclination relative to our line of sight, showing a slightly elongated shape rather than being perfectly circular. There is some evidence of minor disturbances or tidal features in the outer regions of the galaxy, although these features are subtle and require further investigation to confirm.
