The galaxy presents an elliptical morphology, appearing largely smooth and well-rounded. The central region exhibits a concentrated, bright orange-yellow hue, suggesting an older stellar population. There is a slight decrease in luminosity towards the outer edges, which blend gradually into the background. No distinct spiral arm structures or dust lanes are visible. The overall color gradient indicates a possible lack of significant ongoing star formation within the observed timeframe. A very faint and diffuse, slightly blueish object is present on the right side of the galaxy, suggestive of either a star cluster or a small dwarf galaxy at a similar redshift, or potentially a tidal feature.
