The galaxy presents as a centrally concentrated, relatively smooth object. Its overall morphology is consistent with an elliptical galaxy, exhibiting a diffuse, symmetrical structure with no discernible spiral arms or a prominent disk. The core region shows a bright, yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, the color transitions slightly towards redder tones, with the outer regions appearing less defined and more dispersed. There is no evidence of ongoing major merging activity or significant tidal disturbances. The galaxy appears largely isolated in its environment, exhibiting a regular and undisturbed form.
