The galaxy appears to be an elongated, cigar-shaped system. There is a smooth central bulge that seems to dominate the overall structure. Fainter structures or perhaps very faint spiral arms are visible at either end of the elongated shape, giving it an overall length of roughly 3.3 kpc. The galaxy exhibits a blueish hue, suggesting the presence of some young stars and ongoing star formation, although the estimated low star formation rate suggests this is not prolific. There is no obvious evidence of any major ongoing merger activity, although there is a hint of minor disturbance in the overall form. The galaxy shows a relatively smooth overall texture, with a high fraction of light coming from a smooth component as opposed to distinct features like spiral arms or star clusters.
