The galaxy presents an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. Its light profile suggests a central bulge that is relatively bright and concentrated, gradually fading towards the outer regions. The color appears redder towards the core, which could indicate an older stellar population. There appears to be a slight tidal tail or possible merging galaxy on its right side. The overall light distribution seems consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy at a moderate redshift.
