The galaxy presents as a relatively compact object. It appears to be a spheroidal galaxy with a high degree of central concentration. The light distribution suggests a smooth profile. It exhibits a relatively homogenous color, with bluer hues in the center gradually transitioning to slightly redder tones in the outer regions. The image suggests a galaxy in the mass range of approximately 10^10 solar masses. There is evidence of ongoing star formation activity, but it is not particularly vigorous, and it shows signs of past or current merger activity.
