The galaxy presents as a somewhat amorphous, though generally elliptical, structure with a concentrated central region exhibiting a bright, whitish-blue luminosity, possibly indicating a dense population of relatively young, hot stars or an active galactic nucleus. The outer regions of the galaxy diffuse outwards, showing fainter luminosity with a tinge of red, suggesting an older stellar population. There appear to be no distinct spiral arms or a well-defined disk. The overall morphology suggests a system that is either spheroidal or an elliptical galaxy that might be undergoing a minor interaction or disturbance, given the slight irregularity of the outer regions. The galaxy's integrated light implies a modest mass and a relatively low star formation rate, indicative of a system that is either largely quiescent or has recently experienced a burst of star formation.
