The galaxy presents a generally smooth and rounded morphology, exhibiting a concentrated central region. The light distribution indicates a relatively homogenous stellar population. Based on the color indices, the galaxy appears to be dominated by older stellar populations, although the presence of some bluer regions suggests the possibility of ongoing, though limited, star formation activity. The galaxy does not exhibit a strong spiral structure or any clear signs of a disk component. There are no indications of major mergers, although faint asymmetric features suggest potential minor tidal disturbances, possibly from past interactions. The overall appearance is consistent with that of an elliptical galaxy at moderate redshift.
