The galaxy presents as a relatively compact structure, with a dominant central bulge that appears smoothly luminous. The morphology leans towards elliptical, although a slight distortion or feature extends outwards from the central region on one side. The light distribution suggests a well-defined core with a gradual decrease in surface brightness towards the outer edges, exhibiting a degree of roundness. There's a hint of possible minor interaction or internal disturbance contributing to the asymmetry, but no major merging events are immediately obvious from the image. The galaxy has a faint blue tint that suggests some level of recent star formation activity is ongoing within the galaxy. 
