The galaxy presents as a disturbed system, likely undergoing a merger event. Its overall morphology is elongated and somewhat irregular, deviating significantly from a typical elliptical or spiral structure. A prominent feature is a faint tidal tail extending from the main body. This is indicative of gravitational interactions with another galaxy. Within the central region, there appears to be a concentration of older stars, indicated by the redder hue. Patches of bluer light are present as well, suggesting ongoing or recent star formation. The lack of a well-defined disk structure and the disturbed morphology suggest a system where major disruptive processes are at play.
