The galaxy presents as a centrally concentrated system with a smooth, diffuse morphology. There is a lack of discernible spiral arm structure or prominent dust lanes. The central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter with a slight blueish tint. Overall, the galaxy appears somewhat elliptical, though without a distinct axis. There is no obvious interaction with other galaxies or signs of significant tidal disturbance. The overall appearance suggests a galaxy transitioning from a spiral to an elliptical galaxy.
