The galaxy appears as a relatively smooth object, with a roughly elliptical shape. The light profile suggests a concentrated central region, possibly a bulge. There is minimal evidence of spiral arms or a disk structure, indicating the galaxy is likely an early-type galaxy. Its color is mostly a yellow-orange hue, indicative of an older stellar population, suggesting reduced ongoing star formation activity. Faint blue regions may indicate small populations of younger stars. There is no obvious sign of tidal disturbances or interaction with other galaxies. The overall appearance is consistent with a galaxy that has largely completed its star formation and is evolving passively.
