The galaxy presents a largely smooth and featureless morphology. It appears elliptical in shape, exhibiting a high degree of roundness. The central region of the galaxy displays a higher surface brightness, suggesting a concentrated stellar population or active galactic nucleus. Proceeding outward from the center, the light gradually diminishes, forming a halo or envelope surrounding the core, indicative of a bulge. There is no evidence of spiral arms or prominent dust lanes. The galaxy shows a slight color gradient, shifting from a yellowish core to a bluer hue at the edges. This might suggest that there is a greater presence of younger, bluer stars in the outer regions. Overall, the galaxy is a relatively isolated system without any signs of ongoing major mergers or tidal disturbances, although there is a chance of minor disturbances.
