The galaxy presents as a spiral type, with a discernible disk structure. Two spiral arms are prominent, exhibiting a loose winding pattern. A central bulge is visible, appearing moderate in size compared to the overall galactic structure. There may be a weak bar feature present within the central region. The disk is viewed nearly face-on. There are no major disturbances visible, and the galaxy does not appear to be undergoing a significant merger event, but possibly minor disturbances. The galaxy has a redshift of approximately 0.27, indicating that it is relatively distant. The galaxy displays bluer colors in its disk and spiral arms, potentially indicative of ongoing star formation.
