The galaxy presents as a luminous, relatively symmetrical elliptical galaxy with an apparent smooth morphology. It exhibits a concentrated central bulge and a diffuse halo. Its color indices suggest a stellar population dominated by older, redder stars. There may be a faint disk structure, but this needs further observations for confirmation. The galaxy shows some signs of minor disturbances. No active galactic nuclei (AGN) are clearly indicated, but deeper spectral analysis would be needed to exclude the presence of a low-luminosity AGN. The overall morphology suggests that this system is a moderately massive early-type galaxy with a relatively low rate of star formation.
