The galaxy appears as a flattened, elliptical structure with a bright, concentrated central bulge. The overall color profile suggests the presence of a population of older stars, with a notable concentration of these stars in the central bulge. A faint, bluish halo surrounds the central region, indicating the presence of some younger, hotter stars. The disk component appears relatively smooth, with little evidence of prominent spiral arms or distinct star-forming regions. Some minor morphological disturbance seems apparent upon closer inspection around the rim of the galaxy, but is not clearly a sign of merging.
