The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile is centrally concentrated with a gradual falloff towards the outer regions. The core appears bright, exhibiting a yellowish-white hue, suggesting a population of older stars. The overall color gradient across the galaxy shifts slightly towards redder tones in the outer regions, which also hints at an older stellar population with less active star formation. There is no distinct evidence of spiral arms or prominent dust lanes within the galaxy’s structure as depicted in this image. The overall impression is of a galaxy that has largely completed its major star formation phase and is now evolving passively.
