This galaxy presents as a single, relatively smooth object with a high degree of central concentration. The light profile appears largely elliptical, suggesting a classification towards the early-type end of the Hubble sequence. The galaxy's core exhibits a yellowish-white hue, indicative of an older stellar population and reduced levels of on-going star formation. Moving outwards from the core, the galaxy gradually fades into a more diffuse halo with a slightly redder tint, which may be due to the presence of dust. No distinct spiral arm structures or significant tidal features are observable, implying that it is a relaxed system, without signs of recent mergers or major interactions. The overall morphology suggests an evolved system dominated by old stars.
