This galaxy presents a predominantly smooth and elliptical morphology. The central region exhibits a high concentration of luminosity, appearing nearly spheroidal and intensely bright, suggesting an older stellar population. Fainter, more diffuse light extends outwards from the center, forming a halo-like structure. There is a slight asymmetry in the outer regions, possibly indicative of a minor tidal interaction or past merger event. One faint point source appears offset to the right side of the central region. The overall color profile suggests a redder hue throughout the structure, typical of galaxies with low star formation rates.
