The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, almost unresolved point of light, suggesting a high concentration of stars or potentially an active galactic nucleus, though further spectral analysis would be required to confirm this.

Surrounding the core, there is a more diffuse, elongated halo of light that gradually fades into the background sky. The color of the galaxy appears generally blue-white, indicative of ongoing or recent star formation. There is no clear evidence of distinct spiral arms or prominent dust lanes, supporting the classification of an elliptical galaxy.

There are subtle indications of minor irregularities or disturbances in the outer regions of the galaxy, which could be indicative of past interactions or minor merging events. The overall impression is of a massive galaxy exhibiting features consistent with both aged stellar populations and recent star-forming activity.
