The galaxy exhibits an overall smooth morphology, suggesting a relatively undisturbed structure. Its shape appears elongated, tending towards an elliptical form rather than a perfect sphere. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. There is little indication of spiral arms or significant dust lanes. The galaxy appears to be undergoing minimal star formation activity, with no prominent regions of intense blue light indicative of young, hot stars. A slight asymmetry can be observed in the outer regions. Faint tidal features may be present, suggesting a possible past interaction with a smaller galaxy, though further investigation would be needed to confirm this.
