The galaxy presents a generally smooth morphology. The central region exhibits a concentrated, bright, yellowish-orange hue, potentially indicative of an older stellar population and/or dust obscuration. A subtle, less pronounced extension or halo of a dimmer, slightly redder tint surrounds this core, gradually fading into the background. There is no prominent disk structure or spiral arm features visible. A slight irregularity can be seen, but this does not indicate any major merger activity. The overall structure appears relatively undisturbed, suggesting a lack of recent major interactions or significant star formation. The apparent size is small, but given the determined redshift, the galaxy is not small in size.