The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The central region displays a yellowish-white hue, indicating an older stellar population likely dominated by evolved stars. Moving outward from the core, the color transitions to a bluer shade, hinting at the presence of a younger, though potentially still relatively low, population of stars or ongoing, albeit subdued, star formation activity. The overall shape suggests the galaxy is neither perfectly spherical nor highly elongated, showing an intermediate ellipticity. There is no obvious evidence of a distinct disk component, spiral arms, or ongoing major mergers. Faint asymmetric disturbances may be present in the outer regions, potentially indicative of minor interactions. 
