The galaxy appears as a singular object. It displays a primarily smooth morphology, with a slight elongation to its shape, tending toward an in-between, non-distinct form rather than a perfectly round or cigar-shaped structure. There is little apparent disturbance or sign of mergers, indicating relative gravitational stability. The color profile suggests a dominance of older stellar populations, exhibiting a reddish to yellow hue. The galaxy has a fairly small apparent size, but this may be due to the galaxy being relatively far away.
