The galaxy presents as a generally smooth, elliptical structure. Its core exhibits a concentrated, bright yellow-white luminosity, suggesting a high density of older stellar populations. Moving outward from the center, the galaxy displays a diffuse halo with a subtle gradient in color, transitioning toward reddish hues. This gradient suggests a potential decline in the age and metallicity of the stellar populations present within the outer regions. There is minimal evidence of any significant disk-like structure or prominent spiral arms. The overall round morphology indicates that it is likely an elliptical galaxy seen at a redshift of approximately 0.1885. There is little to no indication of any ongoing or recent major merger events. The slight color variations observed may be due to mild differences in stellar population or dust distribution within the galaxy.
