The galaxy presents as an elongated object, appearing somewhat cigar-shaped in overall morphology. It exhibits a relatively smooth profile, with a dominant central bulge that shows a blue hue, suggesting the presence of younger stellar populations. There is the suggestion of a disk component, but it is not clearly defined. The structure appears to be undergoing some form of gravitational interaction or disturbance, as it seems to have a slight tidal tail or minor disturbance in its structure. There is a possible sign of low level star formation. The object is relatively small.
