The observed galaxy presents as a somewhat compact object. The core region exhibits high luminosity, appearing nearly uniform in color and intensity, suggesting a smooth central structure. There is a slightly diffuse extended halo surrounding the core, transitioning from bluer hues near the center to redder tones at the periphery. This color gradient may indicate differing stellar populations or dust distributions. The overall morphology leans toward spheroidal, although potential disruptions or minor asymmetries could be present at the edge of the halo. Faint indications of potential tidal features or interactions cannot be entirely discounted.
