The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge. The light profile appears relatively uniform, with a gradual decrease in intensity outward from the core. Color gradients are subtle, with the central region exhibiting a slightly yellowish hue and outer regions tending toward a greener tone. The galaxy is likely at an intermediate redshift, given its apparent size and luminosity. There is a smaller object in close proximity which could be a companion galaxy or the remnants of a tidal interaction. Overall, the galaxy's features point toward a system dominated by older stellar populations, with little evidence of significant ongoing star formation. However, the possibility of a merger event cannot be entirely ruled out based on its somewhat disturbed shape. Further spectroscopic analysis would be beneficial to confirm these interpretations and gain more insight into its evolutionary history.
