The galaxy presents as a centrally concentrated, elliptical morphology, with a smooth light distribution lacking distinct spiral arm structures or prominent dust lanes. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. This color gradually fades into a bluer periphery. The galaxy's overall shape is elongated, with an apparent axis ratio that indicates a significant degree of flattening, though the possibility of its being a spiral galaxy seen nearly edge-on cannot be definitively ruled out based solely on this image. There are no obvious signs of tidal disturbances or ongoing major mergers.
