The galaxy appears as a relatively compact and luminous object. Its morphology suggests a predominantly smooth structure, with a high degree of circularity. There is little visual evidence of significant spiral arms or a pronounced disk component. The color profile indicates a concentration of older stellar populations, exhibiting a yellowish-orange hue, particularly within the central regions. There are no signs of on-going major mergers or significant tidal disturbances affecting the galaxy's overall structure. The galaxy appears as an isolated system. Overall, the galaxy presents a somewhat elliptical appearance, although not perfectly spherical.
