The galaxy presents as a single, relatively smooth object. It appears elliptical or possibly a lenticular galaxy seen nearly face-on. There is no discernible spiral structure or prominent disk. The color profile suggests a evolved stellar population, exhibiting a yellowish-orange hue. This may indicate older stars and a lower rate of current star formation. There is no evidence of any significant tidal disturbances or ongoing major mergers. There is a slight asymmetry in the light distribution. Overall, the galaxy seems to be a relaxed, relatively undisturbed system, possibly transitioning towards a passive, red-sequence galaxy.
