The galaxy presents as a somewhat flattened elliptical shape, with a relatively smooth overall appearance. Its central region exhibits a bright, concentrated core of light, possibly indicative of a supermassive black hole or dense stellar population. Moving outward from the core, the light intensity gradually decreases. The color profile suggests a mix of stellar populations. The core exhibits a slightly redder hue, which could indicate the presence of older, redder stars, while the surrounding regions show a slightly bluer tint, potentially indicating the presence of younger, hotter stars or some star formation activity. There is a subtle hint of a disk-like structure. No obvious spiral arms or major disturbances are apparent. The galaxy's form suggests it is in a relatively evolved state, with a quiescent morphology.
