The galaxy presents as a moderately luminous object at a redshift of approximately 0.25. It appears predominantly smooth in morphology, exhibiting an elliptical or spheroidal shape, with a relatively high degree of roundness. There is a slight indication of a weak disk-like structure, but no clear spiral arm features are discernible. The galaxy’s color suggests a population dominated by older stars, with a redder overall hue. There is only slight evidence of more active star formation. The galaxy does not appear to be undergoing any major merging events, although there may be evidence of minor disturbances or a past merger event. It has a stellar mass of approximately 10^11 solar masses.
