The galaxy in the image presents a largely smooth morphology, suggesting characteristics of an elliptical or lenticular galaxy. It exhibits a concentrated central bulge with a radial gradient in surface brightness. The core appears bright and lacks substantial internal structure. The overall color profile suggests an older stellar population with a relatively lower rate of ongoing star formation activity. The isophotes indicate it is mostly round, although there are slight deviations that could point to minor tidal interactions or internal asymmetries. Evidence of a prominent disk is not apparent. There do not appear to be significant signs of recent or major merging events.
