This galaxy presents a somewhat smooth, elliptical morphology. Its core exhibits a concentrated luminosity, transitioning to a less defined, more diffuse halo. There appears to be some color variation throughout the galaxy, with the central region having a slightly redder hue while the outer edges have a bluish tinge. This could indicate regions of differing stellar populations or dust content. There is no apparent spiral structure or bar visible. It appears mostly isolated, showing no clear signs of interaction or merging with other galaxies. The overall appearance suggests a galaxy with a moderate degree of star formation, though not exceptionally active.
