The galaxy presents as a relatively smooth, elliptical structure. A bright, concentrated core is clearly visible, suggesting a high density of stars in the galactic nucleus. Moving outwards from the center, the light gradually fades, indicating a decreasing stellar density with increasing radial distance. The overall color appears slightly blue, more indicative of a stellar population that is middle-aged as opposed to an old, redder stellar population. There is no apparent spiral arm structure or distinct dust lanes. The galaxy exhibits a modest degree of roundness, appearing somewhere in between a perfectly spherical and elongated shape. There are no immediately obvious signs of significant tidal disturbances or ongoing merger events. The general morphology suggests a galaxy that is not experiencing intense star formation at the present epoch, and may be transitioning or has already transitioned to a more quiescent state.
