The galaxy presents as a centrally concentrated, luminous spheroid with a smooth, diffuse morphology. There is minimal evidence of spiral arm structures or prominent dust lanes. The color profile suggests a dominant population of older stars. The central region is the brightest and appears to be a yellow-orange hue. A faint, extended halo surrounds the central region, appearing slightly bluer in color. This bluer color may indicate some ongoing, though limited, star formation, although this could also be an artifact of the color imaging process or contamination in the imaging. The overall roundness of the galaxy is very pronounced. No major tidal disturbances are evident.
