The galaxy appears as a compact object, approximately circular in projection. The core exhibits a bright, relatively smooth distribution of light. Surrounding the central region is a more diffuse halo of light, less concentrated than the core. There is a slight hint of asymmetry or minor disturbance in the outer regions of the halo. The galaxy does not exhibit clear spiral arm structures or a well-defined disk component, which would classify it as likely an elliptical galaxy. There is no definitive evidence of a major ongoing merger event; however, slight irregularities could indicate minor interaction with another galaxy or a past merger event.
