The galaxy presents as a slightly elongated, somewhat irregular structure with a dominant smooth appearance. A central bulge or core is suggested, exhibiting a concentration of light. Faint extensions or arms may be present, but these are ill-defined. The light is mostly in the green-red bands, which indicate a mixed population of relatively young and old stars. There is no significant dust obscuration observed. Overall, it resembles an elliptical or lenticular galaxy at an intermediate redshift. The galaxy shows no signs of merging activity or major disturbances and exhibits a low star formation rate.
