The galaxy exhibits a morphology suggestive of an early-type spiral or a lenticular galaxy. It presents with a bright, concentrated central bulge, that gradually diminishes into a faint disk. The disk component appears relatively smooth, lacking prominent spiral arm structures, with the exception of some very faint arm-like features. There are signs of minor gravitational disturbances or interactions that are likely not part of the main galaxy's structure. The galaxy's light is somewhat reddened and could indicate the presence of older stellar populations. Its apparent size is small, indicating its distance, as confirmed by its redshift.
