The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core with a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a bluer tint within the galactic disk, possibly indicating younger stars or ongoing star formation in these regions. The galaxy exhibits a mild degree of asymmetry and some minor disturbances in the outer disk, possibly caused by a minor interaction or internal processes. The overall structure appears relatively well-defined with no signs of a major ongoing merger. The galaxy exhibits a moderate size relative to other galaxies at a similar redshift.
