The observed galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy due to its morphology. Its color appears reddish, indicating an older stellar population with a lower rate of star formation, dominated by redder stars. There is no apparent spiral structure or prominent dust lanes visible in the image. The galaxy shows no signs of major disturbance, suggesting it is not undergoing a major merging event. There appears to be 2 small objects nearby the central galaxy, suggesting this galaxy may be in the process of merging with one or two very small galaxies.