The galaxy presents as a relatively smooth, centralized structure. Its overall morphology appears elliptical, with no discernible spiral arms or strong disk features. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus or bulge. There is an indication of a faint disk.

There are color gradients present across the galaxy. The central regions are a yellow to reddish color, possibly indicative of an older stellar population or dust obscuration. Progressing outwards from the center, the color shifts towards bluer hues. This could be related to younger stars in the outer regions of the galaxy. 

There is no strong evidence of ongoing major merger activity or significant tidal disturbances. The galaxy appears to be in a relatively settled state.
