The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core is bright and exhibits a yellowish hue, suggesting an older stellar population. The isophotes appear regular and concentric, with no strong evidence of spiral arms or a prominent disk. The galaxy exhibits a relatively compact structure, with a gradual fading of light intensity from the center outwards. There is no obvious evidence of ongoing major mergers or significant tidal disturbances affecting the system's overall morphology. Faint blue colors can be detected at the edges of the galaxy.
