The galaxy presents a generally elliptical morphology, appearing relatively smooth and featureless at this resolution. Its central region exhibits a concentrated luminosity, characterized by a yellowish hue. Moving outwards from the core, the color gradually transitions to a bluer shade in the surrounding areas. There's a suggestion of a disk-like structure, but this is not pronounced. The galaxy does not display obvious signs of strong tidal interactions or recent major merger events. However, subtle asymmetries or minor disturbances might be present within its overall structure, warranting further investigation with higher resolution data. The overall color profile suggests the presence of both older stellar populations in the core and potentially younger stars in the outer regions, indicative of ongoing or recent star formation activity at a low rate.
