The galaxy appears as a relatively smooth, elliptical-shaped object with a concentrated central bulge. Its light distribution suggests a fairly uniform stellar population with little evidence of distinct spiral arms or dust lanes. The color is predominantly bluish-white near the core, indicating a population of younger, hotter stars. Moving outward from the center, the color transitions to a slightly redder hue, possibly indicating an older stellar population. There's no obvious sign of active star formation regions or significant irregularities in its morphology, which could be indicative of merger activity. Overall, the galaxy seems to be a well-formed, undisturbed system with a relatively quiescent nature.
