The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. Its overall shape is quite round. The galaxy exhibits a dominant central bulge with a concentrated brightness profile, suggesting an evolved stellar population. There is no evident spiral structure or significant dust lane obscuration. There is a hint of possible minor gravitational disturbance nearby, which could suggest a low possibility of a minor merger event with a dwarf galaxy. The object displays a color profile skewed towards the redder end of the spectrum, typical of elliptical galaxies at intermediate redshifts. Overall, the object is likely an elliptical galaxy with a moderate redshift.
