The galaxy presents as a somewhat elongated, lenticular-like structure. It exhibits a generally smooth morphology, with a noticeable lack of distinct spiral arm features. The central bulge region appears relatively prominent and well-defined. The overall color profile suggests a relatively evolved stellar population, leaning toward the redder end of the spectrum. There is little evidence of active star formation visible within the galaxy, and no indications of recent merger activity or significant tidal disturbances. The light distribution gradually decreases from the center outwards, indicating a substantial but not extremely large size for a galaxy at its approximate redshift.
