The galaxy appears to be a relatively faint object with a subtle, elongated morphology. Its overall color is a pale, slightly bluish-white, which may suggest some ongoing star formation, although a significant portion of the light is likely from an older stellar population. The light is concentrated towards the center.

There is a possible disturbance or minor asymmetry present in the galaxy's outer regions, although it's difficult to distinguish due to the faintness of the galaxy and potential background noise. This may be evidence of a recent or ongoing minor interaction or merger.

Overall, the galaxy does not display prominent spiral arms or a distinct disk structure.
