This galaxy appears to be in a state of merging or significant interaction with another galaxy, or galaxies. There are clear morphological disturbances observed. A prominent feature is a bright central bulge, which is slightly elongated. Extending from this bulge is a fainter, more diffuse halo of light. The overall shape of the galaxy is neither perfectly elliptical nor spiral, showing asymmetry and irregular features. A tidal tail or stream of stellar material is possibly visible, extending to the bottom of the image. Patches of what could be enhanced star formation or disturbed dust lanes are indicated by variations in color and brightness away from the central core, likely associated with the ongoing interaction. The color appears to be somewhat redder in the central regions, which may indicate an older stellar population, with bluer, more irregular regions in the outskirts suggesting more recent star formation activity driven by the interaction. 
