This galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, with a high degree of radial symmetry. The color profile indicates a dominant population of older stars, suggested by the redder hue concentrated in the galactic core. Fainter, bluer hues surrounding the core may indicate ongoing, but relatively low levels of star formation. There is no strong evidence of spiral arms, bars, or other pronounced disk-like structures. The overall light distribution suggests a spheroidal galaxy, potentially an elliptical or lenticular galaxy viewed close to face-on. There is a subtle hint of minor gravitational disturbance in the outer regions, though not enough to make a conclusive statement about any ongoing or recent merger activity.
