The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. Its overall shape is elongated, appearing cigar-shaped. The color profile suggests a dominant population of older stars, with a yellowish-red hue concentrated towards the center and gradually fading towards the outer edges. There's no apparent spiral arm structure or significant dust lanes visible. The overall appearance indicates that the galaxy is not undergoing significant star formation activity and is likely a relatively massive galaxy. There appears to be no major or minor disturbances to the galaxy from external forces, such as merging.
