The galaxy appears to be a somewhat amorphous structure, exhibiting a relatively faint and diffuse morphology. The light distribution suggests neither a perfectly smooth elliptical shape nor a well-defined spiral structure, but instead shows some irregular features. A subtle disk-like structure may exist, but the presence of disturbances prevents clear classification. There appears to be some evidence of recent or ongoing interactions or minor merging events contributing to its irregular shape. The galaxy possesses both blue and redder components of starlight. The overall color suggests the presence of both older stellar populations and some recent star formation activity. The image shows a few distinct, reddish regions, possibly indicating areas of dust obscuration or the location of older, redder stars.
