The galaxy exhibits a relatively smooth morphology, suggesting it is likely an early-type galaxy. The object has a central, bright nucleus indicative of a high concentration of stars in the galactic bulge. It also appears somewhat rounded in shape.

There is evidence of a possible tidal tail or plume extending from the main body of the galaxy. This feature could signify past or ongoing interaction or merging with a smaller object, although it could also simply be an internal phenomenon such as an irregular arm. The object is distorted from a perfect elliptical or spherical shape. There seems to be a minor disturbance to the structure of the object.
