The galaxy exhibits an elongated, cigar-like morphology. It appears to be a relatively smooth system, with a concentrated central region that is yellowish. Fainter, bluer emissions extend along the primary axis of the galaxy, giving the appearance of a disk. There is no apparent ongoing major merger event; the overall structure seems relatively undisturbed. There is also a slight indication of minor disturbance or an interaction, though this is not obvious. The color profile indicates that the galaxy consists of both older stellar populations in the center, and a more moderate star formation rate within the extended disc. 
