The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness. There is little evidence of significant spiral arm structure or a prominent disk. The galaxy's light profile suggests a gradual decrease in intensity from the core outwards, without any clear signs of major disturbances or ongoing mergers. The color profile indicates a relatively homogenous stellar population, with a slight redder hue in the outer regions compared to the brighter, more central areas. Overall, it presents as an early-type galaxy, likely an elliptical or lenticular type, without noticeable features indicative of recent star formation or interactions.
