The galaxy appears to be an elongated, elliptical-like structure with a smooth, relatively featureless morphology. The light distribution suggests a central bulge that is brighter and denser than the surrounding disk. There is a color gradient; the core exhibits a yellowish hue, potentially indicating an older stellar population or a higher concentration of dust. The outer regions of the galaxy appear bluer, which could indicate regions of more recent star formation, although the smooth morphology suggests that star formation is not a dominant process. The galaxy does not appear to be undergoing any major interactions or mergers based on the lack of tidal tails or significant disturbances. It appears isolated or with a smaller dimmer object in the same field of view, so it might be interacting with the galaxy, but this is difficult to assess without further observation.
