The galaxy presents as a moderately bright, diffuse object, exhibiting a roughly elliptical morphology. Its overall color profile suggests a relatively evolved stellar population, with light output peaking towards the redder end of the spectrum. There is a suggestion of a disk-like structure, but this is not sharply defined. Internal features appear subtle, potentially indicating a relatively quiescent star formation rate across the galaxy. There may be a faint tidal tail. No sign of strong spiral arms are present, lending support to the notion of a more relaxed morphology. There is no obvious active galactic nucleus.
