The galaxy presents as a system with a concentrated central bulge, exhibiting a smooth luminosity profile. The morphology is somewhat elliptical, displaying a high degree of roundness. There is a strong color gradient from the center outwards, where the central region displays redder hues, transitioning to yellower tones in the outer regions. There is a suggestion of a minor disturbance within the morphology of the galaxy, perhaps indicating a past or ongoing interaction or merger event. The estimated size of the galaxy is approximately 6 kpc in radius. The overall appearance is that of a relatively quiescent galaxy with an estimated stellar mass on the order of 10^10 solar masses and a low star formation rate. 
