The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing almost spheroidal. The light profile decreases gradually from the core outwards, with no distinct spiral arms or bar structures visible. The galaxy's color gradient is relatively subtle, shifting from a yellowish-white in the center to a slightly redder hue in the outer regions. There is no clear evidence of significant dust lanes or recent major merger activity disrupting the overall smoothness of the galaxy’s structure. Faint hints of irregularities could suggest minor tidal interactions or disturbances, but the dominant impression is one of a relaxed, evolved system.
