The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity, gradually decreasing towards the outer edges. There's an apparent lack of distinct spiral arms or a well-defined disk. Coloration suggests a slightly redder core region, which could imply an older stellar population dominating the center, with bluer colors faintly present in the galaxy's outskirts. The galaxy's shape is roughly circular. There are no obvious signs of ongoing major mergers or significant tidal disturbances in this image.
