The galaxy presents an overall smooth morphology, appearing as a diffuse, centrally concentrated structure. Its shape is generally elliptical, exhibiting a slight deviation from perfect circularity. The core region displays a luminous, yellowish hue, suggesting a population of older stars.  The light intensity gradually decreases from the center outwards, with the outer regions exhibiting subtle color variations, possibly indicative of varying stellar populations or dust distribution. There is little evidence of distinct spiral arms or a prominent disk structure.  No significant signs of major mergers or tidal disturbances are apparent.