The galaxy presents a relatively smooth and concentrated appearance. The primary body of the galaxy exhibits a yellowish-white hue, suggesting an older stellar population. A distinct reddish region is observed, which could indicate dust obscuration, ongoing star formation activity, or a combination of both. The galaxy does not appear to have a clearly defined spiral structure. There is a possibility of a minor interaction or merger event occurring, given the slightly disturbed morphology of the galaxy. The galaxy’s overall shape is generally round, with a slight deviation towards a more elliptical form.
