The galaxy presents as an elliptical morphology, appearing cigar-shaped due to its high ellipticity and exhibiting a smooth light distribution. There is no obvious presence of spiral arms or a prominent disk. The color profile suggests a predominantly older stellar population, based on its redder hues. Signs of active merging events or major disturbances are minimal. It is at an approximate distance of 215 megaparsecs, based on its redshift of 0.050287. The galaxy is estimated to contain a stellar mass of approximately 2.25 x 10^9 solar masses.
