The galaxy presents as a single, coherent object with a smooth, elliptical morphology. It exhibits a noticeable concentration of luminosity towards its center, suggesting a prominent bulge. The color profile transitions gradually from a yellowish-white core to a redder outer halo, indicating a potential shift in stellar populations from older stars in the central region to a mix of older and possibly some younger stars in the periphery. There is no discernible spiral arm structure or any significant dust lane obscuration. The overall impression is that of a relatively evolved galaxy, possibly an elliptical or lenticular type. No clear signs of active galactic nuclei or recent major mergers are evident in this image. There is a slight asymmetry to the galaxy's overall shape, but it seems generally spheroidal.
