The galaxy presents a somewhat disturbed morphology, possibly indicative of an ongoing or recent interaction. Its overall shape is not perfectly elliptical, displaying a deviation towards a more elongated form. There is an apparent tidal tail or plume extending from the main body of the galaxy. This plume exhibits a bluer color, suggestive of recent star formation activity within it. The central region of the galaxy exhibits a yellowish hue, indicative of an older stellar population dominating this area. The bulk of the galaxy appears relatively smooth, however some features seem to be present that can be further investigated. These features could be due to ongoing star formation or dust obscuration.
