The galaxy presents as an elongated, cigar-shaped structure. There is a prominent central bulge that appears reddish-orange in color, suggesting an older stellar population dominated by redder stars. The surrounding disk, while not sharply defined, shows hints of bluer regions, possibly indicating areas of more recent star formation. Overall, the galaxy appears relatively smooth, with no obvious signs of major disturbances or mergers. There is some evidence of slight asymmetry in the outer regions of the disk. The galaxy is likely a spiral galaxy.
