The galaxy appears to be a somewhat diffuse object with a centrally concentrated luminosity profile. A discernible disk structure is not clearly present within this image. The galaxy's core region exhibits a brighter, more compact morphology, implying a concentration of stellar populations or a potential active galactic nucleus.

Hints of disturbance are present in the galaxy's outer regions. These appear in the form of slight asymmetries or faint tidal features, suggesting past or ongoing gravitational interactions. While the majority of the galaxy's light appears relatively smooth, a subtle feature disrupts the smoothness. The galaxy shows a blue tint indicating possible star formation and is brighter in the green wavelengths of the spectrum than red, but these are not pronounced.
