The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish core to bluer outer regions. This suggests older stellar populations are concentrated towards the center, while the outskirts may contain more recent star formation activity. There is no evidence of a prominent disk structure or spiral arms. Subtle irregularities in the outer regions may indicate minor tidal interactions or past accretion events, but the overall structure appears relatively undisturbed. The galaxy appears to be significantly massive. Star formation is present, but at a moderate level.
