The galaxy presents a relatively compact structure. It is an oblate spheroid, appearing as a flattened disk when viewed from our vantage point. There is a bright, concentrated core suggesting a high density of stars and possibly an active galactic nucleus.

Surrounding the core, there is a defined region of lower surface brightness. This area appears relatively smooth, lacking prominent spiral arm structures or distinct features. The color distribution indicates a slightly bluer hue in the outer regions, implying younger stellar populations compared to the core.

There is a faint indication of possible tidal disturbances or minor irregularities in the galaxy's morphology. The asymmetry could indicate an ongoing or past merger event, though the dominant impression is of a system that is relatively undisturbed. Overall, the galaxy exhibits characteristics consistent with a disk galaxy transitioning to a lenticular classification.
