The galaxy presents as an elliptical morphology, exhibiting a smooth and largely featureless light distribution. The central region displays a high concentration of light, appearing a yellowish-orange hue. Moving outwards, the light gradually diminishes in intensity, with the outer regions exhibiting a subtle greenish tint, possibly indicating the presence of a faint, extended stellar population or ionized gas. The overall shape is elongated, with a moderate ellipticity. There's no obvious presence of spiral arms, dust lanes, or other distinct morphological features typically associated with spiral galaxies. No clear evidence of a major ongoing merger is visible, though a subtle asymmetry cannot be entirely ruled out. The galaxy's structure suggests it is a relatively evolved system, likely dominated by older stars and potentially a supermassive black hole at its center.
