The galaxy presents as a centrally concentrated spheroid with a smooth overall appearance. A pronounced central bulge is observed, exhibiting a yellowish hue, likely indicating an older stellar population. A slightly flattened disk component surrounds the bulge, displaying a bluer color, suggesting the presence of younger stars and ongoing star formation. The outer regions of the galaxy fade gradually into the background, indicating a low surface brightness halo. There are no clear signs of spiral arms or prominent dust lanes. Minimal disturbance to the system.
