The galaxy presents a largely smooth and rounded morphology. The light distribution appears centrally concentrated with a noticeable decline in surface brightness moving outward from the core. The color gradient suggests an older stellar population dominating the galaxy's overall emission. There is little evidence of significant dust lanes or spiral arm structures, indicating a relatively quiescent star formation history. No major merger events are apparent. The galaxy is most likely an elliptical galaxy, possibly a lenticular galaxy.
