The galaxy presents as a somewhat smooth, centrally concentrated object. It is characterized by a generally elliptical morphology, although it does exhibit some noticeable deviation from perfect roundness, appearing slightly elongated. The galaxy is dominated by light in the redder end of the spectrum. There is some asymmetry and potential for minor tidal disturbances. These disturbances suggest possible past or ongoing gravitational interactions. At its estimated distance, this galaxy spans several kiloparsecs in diameter and contains a substantial amount of stellar mass. The specific star formation rate suggests that the galaxy is currently undergoing only a modest amount of star formation activity.
