The galaxy presents a generally elliptical morphology. Its central region exhibits a concentrated luminosity, appearing as a bright, amorphous core. Moving outwards from the center, the intensity of light diminishes, and the galaxy's overall structure appears largely smooth. There are subtle color gradients observable, with a possible slightly bluer central hue transitioning to a more neutral color in the outer regions. While no distinct spiral arms or well-defined structures are immediately apparent, there appears to be some minor irregularity in the outer halo. The galaxy's light distribution suggests it is relatively compact. No clear signs of major interaction or ongoing merger events are detectable in this image, but there might be a subtle disruption of the galaxy's symmetry.
