The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular, showing no significant elongation or asymmetry. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. There is a gradual decrease in luminosity from the center outwards, with no distinct spiral arms or prominent disk-like structure visible. The color profile shows a relatively uniform distribution of light across the galaxy, with a slight yellow-red hue. This indicates an older stellar population, characteristic of elliptical galaxies, with a very low rate of star formation. There are no signs of recent or ongoing mergers, tidal tails, or other disruptive features. The galaxy appears to be relatively isolated and undisturbed.
