This galaxy exhibits a generally smooth morphology, appearing as a flattened, cigar-shaped structure. There is a central, brighter region, suggesting a concentration of stars or perhaps an active galactic nucleus. The color appears somewhat redder overall, with bluer stars scattered throughout the galaxy. There is little to no visible spiral structure or prominent dust lanes, indicating a disk dominated by an older stellar population. There does not appear to be any interaction or merger events presently occurring, but there is evidence of a minor disturbance in the galaxy. It is likely a lower mass galaxy, with a low rate of star formation.
