This galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape is somewhere between round and elongated, presenting a cigar-like profile. While no distinct spiral arm structure is discernible, there is some evidence of a disk component. There is no obvious signs of tidal disruption or interaction with a companion galaxy. The galaxy appears to be emitting light in the green, red, and possibly blue regions. Given the colors, this suggests that the galaxy is relatively massive.
