The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting an elliptical morphology. It shows a notable lack of distinct spiral arms or other readily discernible features typically associated with disk galaxies. The light profile appears to gradually decline from a bright central bulge, suggesting a significant concentration of older stellar populations. Color gradients are subtle, but a slight reddening toward the central regions might indicate an increased density of dust or a higher proportion of older, redder stars. There's a hint of slight disturbance on one side, a subtle asymmetry in the outer halo, potentially indicating the presence of tidal interactions. Overall, the galaxy appears to be an intermediate to massive system, potentially an early-type spiral or elliptical galaxy at a moderate redshift.
