The galaxy presents as a somewhat elliptical, moderately concentrated object. The core region exhibits a high degree of luminosity, appearing almost unresolved in this image. There's a gradual decline in surface brightness moving outward from the center. Hints of disk-like structure are subtly present, but the galaxy is dominated by a smooth, spheroidal appearance. Faint blue tinges are visible in the outer regions, suggesting the presence of some younger stellar populations, but the overall color profile indicates a significant population of older stars. While generally smooth, there's a slight asymmetry detectable in the extended halo, potentially indicating minor tidal interactions or disturbances. It does not present as an active merging galaxy but could have experienced a minor merger event in its past.
