The galaxy presents as a relatively smooth, ellipsoidal structure with an apparent aspect ratio suggesting it is not viewed perfectly face-on. A bulge component is noticeable, exhibiting a concentrated brightness towards the center. The primary color is indicative of an older stellar population. There may be faint evidence of a disk structure. A disturbance in the color gradient is visible at the periphery. The system appears to be isolated with no evident tidal features or nearby companions indicating recent or ongoing major merger activity, though there might be a minor disturbance. The overall morphology suggests a galaxy transitioning towards a more passive, early-type system.
