The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution suggests a relatively high degree of symmetry, with the intensity decreasing gradually from the core outwards. There is a slight elongation. The galaxy exhibits a color gradient, with a bluer hue towards the outer regions and a slightly redder core. The color variation may indicate differences in stellar populations, with younger, bluer stars dominating the outer parts and older, redder stars concentrated in the center. There are no obvious signs of spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies.
