The galaxy presents a generally smooth and elliptical morphology. There is a high degree of central concentration, with the luminosity appearing to decline gradually from the core. A distinct nucleus is not readily apparent. The overall color appears slightly redder, suggestive of an older stellar population. There are no visible spiral arms or bar structures. No signs of any major disturbances or recent merger activity are immediately obvious. There may be a hint of minor asymmetry or faint tidal features in the outskirts, warranting further investigation, but the galaxy generally appears relaxed and well-formed. The galaxy exhibits a fairly round shape.
