The galaxy presents as a centrally concentrated, relatively smooth object with a dominant elliptical morphology. The light profile is brightest and most yellow-reddish at the core, indicating an older stellar population and potentially a supermassive black hole actively emitting radiation. Moving outward from the nucleus, the color appears to trend slightly bluer. This may signify younger star formation. However, given the galaxy's dominant morphology, the amount of on-going star formation is likely low overall, which could explain the overall redder color. There are no visible spiral arm structures. The roundness of the galaxy suggests a classification closer to E0, or perhaps E1 or E2, but it is difficult to assess the exact ellipticity without a clearer, higher-resolution image. There are some slight indications of minor disturbances around the galaxy. Overall, it appears to be relatively isolated and undisturbed, residing in a fairly empty region of space.
