The galaxy presents a largely smooth morphology. The color profile indicates a concentration of older stellar populations towards the center, characterized by a yellowish hue, possibly suggesting a bulge-dominated structure. Fainter, bluer extensions surround the central region, indicating the presence of some younger stellar populations and potential ongoing, but low levels, of star formation in the outer regions. There is no prominent disk or spiral arm structure visible. The shape is approximately round. There's no obvious evidence of any major merger events or tidal disturbances. Overall, this galaxy appears to be an evolved system undergoing relatively quiescent star formation.
