The galaxy presents a largely smooth, elliptical morphology. Its color profile is dominated by a yellow-orange hue, suggestive of an older stellar population with a lower rate of current star formation. The galaxy appears to be relatively isolated with no obvious signs of interaction or tidal disturbances in the surrounding field, which points towards it not undergoing any major merging events recently. The object appears mostly rounded in shape, with no bar or obvious spiral arms, suggesting it is classified as an elliptical galaxy. The size of the galaxy appears relatively small, corresponding to a moderate physical size at its redshift, indicating it is a dwarf or intermediate-sized galaxy. Overall, the galaxy exhibits characteristics consistent with a passively evolving system.
