The galaxy appears as a centrally concentrated object with a smooth morphology. It exhibits an elongated shape, with an aspect ratio suggesting it is likely an elliptical galaxy. The core presents a bright, concentrated luminosity, gradually diminishing outwards. The color profile indicates a primarily older stellar population, with a redder hue towards the center that fades to a bluer color in the surrounding regions. The absence of spiral arms or other distinct features suggests a lack of ongoing, large-scale star formation within the disk. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. It is a fairly isolated galaxy with no other large bodies nearby.
