The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. Its color gradient suggests a concentration of older stellar populations towards the galactic core, with the central region presenting a yellowish-orange hue. Fainter, diffuse light extends outwards from the core in a roughly elliptical shape, indicative of a spheroidal component. There is a subtle hint of bluer colors in the outer regions, potentially suggesting some ongoing, though modest, star formation activity in the galaxy's periphery. No distinct spiral arm structures or prominent dust lanes are discernible at this resolution. Overall, the galaxy presents the appearance of a fairly evolved system, possibly an elliptical or lenticular galaxy, with a dominant bulge component.
