The galaxy appears to be a spiral galaxy with a redshift of approximately 0.122. It displays a bright, prominent central bulge, suggestive of an older stellar population. A faint and tightly wound spiral structure extends from the bulge, primarily visible on the left side. The galaxy exhibits an overall elliptical morphology. The spiral arms display a bluer color, indicating the presence of younger, hotter stars and regions of ongoing star formation. The outer regions of the galaxy are diffuse and less defined, with a slightly flattened appearance. Some evidence indicates the presence of minor tidal disturbances.
