The galaxy presents as a concentrated, centralized structure. Its form is generally smooth, lacking prominent spiral arms or a distinct disk. The luminosity appears relatively even across the galaxy's body, with a slight concentration towards the center.  There is a hint of asymmetry or possible disturbance, suggesting a subtle tidal interaction or minor merger event. The central region shows a somewhat spherical morphology, but appears slightly elongated. There's a slight blueish tint in some of the outer regions of the galaxy. The galaxy's shape is somewhere between round and elongated, but favors the rounder end of the spectrum.  There is no clear evidence of a major merger.
