The galaxy presents as a moderately luminous object at a considerable distance, inferred from its redshift. Morphologically, it exhibits a somewhat smooth appearance, although there is subtle evidence of a disk-like structure or features within the galaxy's central region. The overall shape is neither perfectly spherical nor highly elongated, appearing to be an intermediate elliptical galaxy. The galaxy displays a predominantly yellowish-orange color gradient, with a possible faint trace of blue in the periphery. There are suggestions of some gravitational interaction or disturbance, with a faint plume extending from the primary body of the galaxy, hinting at potential minor merger activity. Based on its color profile, it could be inferred that the galaxy contains a relatively older stellar population, but the presence of a disk-like structure points to some ongoing, even if mild, star formation.
