The galaxy appears to be a relatively smooth, elliptical system. Its core exhibits a bright, concentrated luminosity, gradually fading outwards. There is very little evidence of distinct spiral arms or a prominent disk structure. The overall shape is largely round. The color profile suggests a population of older stars, with a general reddish-yellow hue dominating the central region. There are no clear signs of ongoing major mergers or significant tidal disturbances. The outer regions show a more diffuse and indistinct structure, with a subtle transition to the background sky.
