The galaxy presents as an elliptical morphology, appearing somewhat elongated, with a smooth overall structure. Its color profile indicates a dominant redder population, suggesting an older stellar population and/or significant dust extinction. There is no evident spiral arm structure or prominent dust lanes. The galaxy core exhibits higher surface brightness, with light intensity decreasing gradually outwards. No obvious signs of ongoing major mergers or strong tidal disturbances are visible, although minor asymmetries cannot be ruled out at this resolution. The morphology could be classified as an elliptical galaxy of considerable mass.
