The galaxy presents a morphology that is neither distinctly elliptical nor spiral, appearing as a somewhat amorphous structure. Its color profile indicates a significant population of older stars, contributing to a reddish-yellow hue. There is some evidence of bluer regions, suggesting the presence of younger stellar populations, though these are not dominant. 

The overall structure exhibits some disturbance, possibly indicating an ongoing or past minor interaction or merger event. The galaxy appears to be moderately massive with an ongoing rate of star formation. 
