The galaxy presents a generally smooth and elliptical morphology. It is primarily a spheroid-dominated system. The light distribution appears concentrated towards the center, with a gradual decrease in luminosity outwards. A subtle blue hue is observed, suggesting the presence of some younger stellar populations. Faint distortions or a subtle tidal feature appears to extend from the main body of the galaxy, hinting at a possible past interaction or minor disturbance with another galaxy. Overall, the galaxy does not exhibit a prominent disk or spiral arm structure.
