The galaxy presents as a system of closely interacting components. The dominant feature is a large, relatively smooth central component exhibiting a yellow-orange hue. This indicates a population of older stars. Adjacent to this central mass is a second, somewhat less distinct and slightly smaller component, sharing a similar coloration. There appears to be some overlap or tidal interaction between these two main features. 

The overall morphology of the galaxy is somewhat amorphous, lacking a well-defined spiral structure. Some subtle irregularities and faint extensions are observed around the brighter components, which could be indicative of ongoing or recent merger activity. The relatively red colors suggest a galaxy with comparatively low star formation activity.
