The galaxy presents as a relatively compact, smooth object with a bright, concentrated core. The overall shape appears to be generally round, with a slight suggestion of elongation. There is little evidence of distinct spiral arms or prominent features, suggesting a morphology leaning towards an elliptical or lenticular classification. The color profile is dominated by yellow to red hues, implying a stellar population that is predominantly older, with fewer young, hot stars. Any disk is not distinctly resolved. The galaxy shows no visually apparent signs of any major ongoing merger activity or significant tidal disturbances, seeming undisturbed. Given the measured redshift, the light we observe is redshifted, implying that the galaxy is relatively far from us, so some of the finer details of this galaxy can not be seen.
