The galaxy presents as a luminous, centralized object with a generally elliptical morphology, appearing largely rounded in shape. A smooth luminosity profile dominates the galactic structure. The central region exhibits a higher concentration of light, suggesting a prominent galactic nucleus or bulge. Extending outward from the core, a faint halo or extended envelope is visible, gradually diminishing in brightness towards the outer edges. There is a hint of asymmetry or minor disturbance in the outer regions of the galaxy, but no clear signs of ongoing major merging activity are apparent. Color gradients suggest some differential stellar populations, with the central region tending towards a yellower hue and the outer halo exhibiting a slight shift toward a redder tone. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy that appears relatively relaxed and evolved.
