The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated object with a major axis visibly longer than its minor axis. Its light profile indicates a bulge-dominated system, showing a gradual fading of luminosity from the core outwards. The color profile suggests a redder central region transitioning to slightly bluer hues in the outer regions, possibly indicating a change in stellar populations. There's no clear evidence of spiral arms, star formation regions, or a prominent dust lane within the observed image. The overall appearance is consistent with an evolved galaxy exhibiting minimal ongoing star formation.
