This galaxy presents as a concentrated object with a bright, unresolved core. The object exhibits a dominant blue hue, indicative of a younger stellar population and/or active star formation. There is a subtle extension of diffuse light surrounding the bright core, displaying a faint red shift on the outer rim. The morphology appears generally smooth, with only slight evidence of disturbances. Based on the color, the galaxy is likely undergoing interactions and potentially merging with another galactic object, though that is difficult to definitively prove without further data. 
