The galaxy appears to be composed of two distinct components. The primary, larger component exhibits a generally smooth morphology, with a concentrated central bulge. The color is predominantly yellow/orange, suggesting an older stellar population with diminished recent star formation. 

A secondary, smaller component is located nearby. This component is elongated and appears as a faint disk. Its color is shifted towards the red end of the spectrum, potentially indicative of dust or a population of older stars. There is no strong evidence of significant tidal disturbances or ongoing major mergers within the galaxy. 
