The galaxy presents a predominantly smooth morphology, characterized by a centrally concentrated, bright core region that emits strongly in the red and green bands. This core gradually fades into a more diffuse halo. The overall shape appears nearly circular, suggesting a possible elliptical or lenticular classification. There is a minor asymmetry visible, indicating a slight disturbance in the galaxy's structure. This could be due to a past or ongoing minor interaction with another celestial object. No prominent spiral arms or bar features are discernible.
