The galaxy exhibits a spiral structure, as suggested by the presence of prominent, well-defined arms. The spiral arms appear to be winding moderately tightly around the central bulge. The central bulge is clearly visible and constitutes a substantial fraction of the galaxy's overall luminosity and size. The bulge appears somewhat bright, likely indicating a considerable population of older stars. There is evidence of a possible bar-like structure running through the center of the bulge. The disk component of the galaxy appears less prominent than the bulge. The galaxy is tilted relative to the observer's line of sight, presenting an inclined view. The arms display subtle color variations, with some regions exhibiting bluer hues potentially indicative of on-going star formation. There are no obvious signs of a major merger event, though minor disturbances in the disk may be present.
