The galaxy presents with a relatively compact morphology. The central region exhibits a high degree of luminosity, appearing as a bright core. Diffuse light extends outwards from this core, but its distribution is not uniform, with some areas of the galaxy appearing fainter or less defined. A subtle asymmetry can be noted in the light distribution extending from the core. Overall, the object does not exhibit the classic spiral arm structure typically associated with disk galaxies. There might be a faint indication of a disk component contributing to the broader light distribution, but its presence is not definitive from this image. The object may have a relatively smooth overall appearance, with minimal evidence of significant ongoing mergers or major disturbances. 
