The galaxy appears to be an elliptical type, exhibiting a generally smooth, round morphology. The central region displays a concentrated luminosity, suggesting a substantial stellar population. The core color is yellow, possibly indicating a population of older, redder stars dominating the galactic center. There is a hint of a fainter, bluer extended halo surrounding the core, implying the presence of a younger stellar population that might extend beyond the main body of the galaxy. No distinct spiral arms or prominent dust lanes are visible. There appear to be no major disturbances or signs of ongoing mergers affecting its global structure. However, the suggestion of a faint extended halo could indicate some past interaction, depending on the halo's nature. Overall, the galaxy presents a relatively quiescent appearance.
