The galaxy exhibits a discernible spiral structure. Its arms are not tightly wound, indicating a relatively late-type spiral classification. The presence of numerous HII regions, suggested by the clumpy and irregular distribution of brighter regions along the spiral arms, implies active star formation. A bar-like structure may exist at the center of the galaxy, however, it is difficult to determine from the image.

A noticeable bulge component is present, though its size appears moderate relative to the overall galactic disk. There are indications of a possible interaction or recent merger event, with a slightly distorted morphology. The galaxy displays a blueish hue in some regions, indicative of younger stellar populations, while other areas appear redder, suggesting the presence of older stars. The galaxy is likely a spiral galaxy at a redshift of approximately 0.23. The estimated physical size corresponds to a medium-sized galaxy.
