The galaxy presents an overall elliptical morphology, though with some notable irregularities. Its central region exhibits a high concentration of light, appearing as a bright, diffuse nucleus. This central region shows evidence of multiple, less defined light clumps. These clumps may indicate ongoing or recent merger activity, possibly with smaller satellite galaxies.

The galaxy's outer regions display a gradual decrease in surface brightness. There is no readily apparent spiral arm structure or prominent dust lanes. A faint, extended halo or envelope of stars and gas may be present, but this is difficult to ascertain conclusively due to the image's limited resolution.

Overall, the morphology suggests a galaxy that has undergone or is undergoing significant interactions that has disrupted the otherwise smooth symmetry of the galaxy.
