The galaxy presents as an elongated, disk-like structure, viewed at a high inclination. The central region exhibits a brighter, more concentrated luminosity, suggestive of a nuclear bulge. There's a discernible color gradient, with the central bulge appearing yellower, potentially indicating an older stellar population, compared to the bluer, outer regions of the disk which may be indicative of younger stars and ongoing star formation. The galaxy appears relatively smooth with no distinct spiral arm structures evident, although some minor disturbances in the disk's morphology are noticeable. Overall, the galaxy appears to be an edge on spiral or lenticular galaxy, with a dominant bulge and disk component, at a redshift of approximately z = 0.06.
