The galaxy presents as a centrally concentrated object with a largely smooth morphology, indicative of a probable elliptical or lenticular classification. There is a slight asymmetry, potentially revealing some feature or possible minor disturbance in the disk and/or halo. The primary body has a generally rounded shape and appears to be the dominant mass distribution. There are also a number of features which are not as intense in surface brightness.

The galaxy displays a color gradient, appearing bluer in certain regions, possibly tracing more recent star formation activity. These regions appear more distinct than the smoother, redder regions of the galaxy's core. This may suggest ongoing, albeit modest, star formation activity in the outer regions compared to a quiescent core. The overall faintness and relatively small angular size suggests this is a fairly distant object.
