The galaxy appears as a somewhat elongated, cigar-shaped structure. There is evidence of a central bulge, though it appears relatively small in comparison to the overall length of the galaxy. The disk is visible, and its color suggests a mix of stellar populations. The disk appears to be significantly disrupted or undergoing some sort of tidal interaction, based on the deviation from a perfectly smooth shape and the color. The blue-ish light indicates recent star formation. The smooth appearance and general morphology suggests a relatively quiescent galaxy, but there could be minor disturbances. There is no obvious sign of a major merger.
