The galaxy exhibits a moderately inclined disk structure, with a notable central bulge. The bulge appears relatively smooth and concentrated, while the disk shows a more diffuse texture. There are hints of spiral arm structure, though they are not sharply defined. The overall color of the galaxy leans towards the redder end of the spectrum, suggesting a population of older stars and relatively suppressed star formation. There are some subtle asymmetries in the disk's structure, potentially indicating past interactions or mergers. The galaxy displays moderate angular size.
