This galaxy presents a disturbed morphology, suggesting it is undergoing or has recently undergone a significant gravitational interaction. A tidal tail is visible extending from the main body, characterized by a bluer hue indicative of younger stellar populations and active star formation. The primary galactic body is more centrally condensed, with a yellowish-orange core, which may indicate an older stellar population. The galaxy's overall shape is irregular and elongated, deviating significantly from a typical elliptical or spiral structure. There appears to be a secondary, less defined stellar population visible in the tidal stream. Evidence of potential ongoing star formation is seen with the regions of bluer light emanating from the tidal tail. The galaxy appears to be relatively compact, yet still demonstrates notable gravitational interactions.
