The galaxy presents as a spiral type, viewed at a significant angle relative to its galactic plane. There is evidence of spiral arm structure; however, image resolution limits detailed characterization. The central bulge appears moderate in size and exhibits a yellowish hue, indicative of a population of older stars. Fainter, bluish regions are observed extending outward from the bulge, likely associated with regions of ongoing or recent star formation. There is no clear indication of a strong bar structure, although a weak bar cannot be ruled out due to the angle of observation. No major disturbances in the morphology that would suggest a recent major merger are evident, though minor disturbances are possible. Overall, the galaxy appears as a relatively normal spiral galaxy with a redshift of approximately 0.048.
