The galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a bright, yellowish hue, indicating the presence of older stellar populations. Moving outward from the core, the galaxy's color transitions to a slightly redder tone, implying a potential gradient in stellar age or metallicity. While generally smooth in appearance, there's a hint of slight elongation. No distinct spiral arms or well-defined disk structures are immediately apparent in this image, suggesting it may be an elliptical or lenticular type galaxy. There are no obvious signs of major mergers or significant tidal disturbances in this particular view, though minor asymmetries cannot be entirely ruled out given the image resolution. Overall, the galaxy appears to be a mature system.
