The galaxy presents as a roughly elliptical, lenticular form, exhibiting a smooth, primarily featureless morphology in this image. The central region displays a concentration of light, appearing as a bright, slightly elongated core. A subtle color gradient is visible, with the core appearing more yellow-white, transitioning to a bluer hue in the outer regions. This color shift might indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars contributing to the outer luminosity. The lack of spiral arms or significant dust lanes suggests a relatively quiescent star formation history. The overall shape indicates it is not perfectly rounded, but rather somewhat elongated. There is no indication of major tidal disturbances or ongoing mergers, though there might be a slight asymmetry in the outer halo. The galaxy's redshift suggests that it is at a considerable distance from our own.
