The galaxy presents an irregular morphology. There is evidence of a central, somewhat amorphous structure, with diffuse extensions. The color profile suggests ongoing or recent star formation, indicated by bluer tones interspersed within the galaxy. Distinct clumps or knots of higher intensity are visible within the brighter, central regions. The overall structure hints at the possibility of a past or ongoing interaction or merger, disrupting a more regular form. There is a faint tail like feature extending from the galaxy.
