This galaxy presents a generally smooth, elliptical morphology with a central concentration of light. There is a discernible color gradient, with the core appearing somewhat bluer compared to the outer regions, which exhibit a redder hue. The overall shape is slightly elongated but does not show any distinct spiral arm structures or obvious signs of major disturbances. The galaxy appears relatively isolated, showing no strong evidence of ongoing or recent major mergers based on the image data. There is a subtle asymmetry to the light distribution, suggesting a possible minor interaction or internal dynamic process. The estimated size indicates this is a moderately sized galaxy at its redshift.
