The galaxy presents a generally smooth, somewhat rounded morphology. There is a hint of a disk structure, but the overall appearance is dominated by a central bulge or spheroidal component. The light distribution suggests a relatively evolved stellar population, potentially with ongoing, but subdued, star formation activity. There is no clear evidence of major mergers or significant tidal disturbances. A subtle asymmetry can be observed in the outer regions of the galaxy, which could indicate a minor interaction. The galaxy exhibits a redder color, consistent with a relatively high redshift.
