The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated region of bright, blue-white light, suggesting the presence of a significant population of young, hot stars or an active galactic nucleus. The outer regions gradually fade into a less defined halo, with a subtle elongation along a preferential axis. A slight asymmetry in the light distribution may indicate a minor gravitational interaction or disturbance. The overall color profile suggests moderate star formation activity within the galaxy. 
