The galaxy presents as an elliptical structure with a generally smooth appearance. The central region exhibits a concentrated, bright yellowish hue, likely indicating an older stellar population. Progressing outward, the galaxy transitions into a bluer color, suggesting the presence of younger stars and potentially some ongoing star formation, however, the star formation rate appears generally low. The overall shape can be described as somewhat elongated, rather than perfectly spherical. There is no discernible evidence of major mergers or significant tidal disturbances in this image. The absence of strong spiral arm features, together with the smooth central bulge and redder color in the center, reinforces its identification as an elliptical or lenticular galaxy. 
