The galaxy presents as a relatively smooth, single structure, with a mostly rounded appearance. The object has a central concentration of light. This could be indicative of a bulge. There is a subtle color gradient moving outwards. The core of the galaxy is yellowish, while the outer regions appear slightly redder. This gradient suggests possible differences in stellar populations, with the core potentially containing older, redder stars and the outer regions harboring a younger, bluer population. There seems to be slight asymmetry in the shape of the object which could be the result of past interactions or mergers. There are no obvious spiral arms or bar features. The galaxy shows a very subtle halo.
