The galaxy presents a predominantly smooth morphology. The central region exhibits a bright, concentrated core that transitions into a more diffuse, extended halo. There is a hint of asymmetry in the outer regions. Color gradients are apparent, with the core appearing bluish-white, suggestive of hotter, younger stellar populations. The surrounding halo shows a greenish tint, possibly indicating a mix of stellar populations and/or gas emission. No clear spiral arms or distinct features are discernible. There are subtle indications of potential minor disturbances or interactions in the form of slight distortions of the halo, but these are not definitive merging features. Overall, the galaxy's morphology is predominantly smooth, with a bright core and diffuse halo, and subtle hints of possible interactions.
