The galaxy presents as a relatively smooth, elliptical structure, exhibiting a somewhat rounded morphology rather than a highly elongated or disk-like shape. It appears centrally concentrated with a gradual decrease in luminosity towards its outer edges. There's a hint of a redder hue concentrated towards the center, possibly indicating a population of older stars.  A subtle, diffuse blue component is also present, possibly indicating some degree of ongoing star formation. There is potential evidence of a minor disturbance in the galaxy's morphology, suggesting a possible interaction or merger history, however, a substantial portion of its population believes the galaxy is undisturbed.
