The galaxy presents as a somewhat flattened spheroid, elongated along one axis. Its morphology appears relatively smooth, lacking prominent spiral arms or a well-defined disk structure. The central region exhibits a slightly higher concentration of light, suggestive of a galactic bulge. The color profile is subtly redder in the central region, possibly indicating an older stellar population or dust obscuration, with bluer fringes. Overall the galaxy does not appear to be undergoing a major merger, with no obvious tidal tails or signs of significant gravitational disturbance. It appears to be an isolated galaxy with a stellar mass on the higher end of the scale.
